Because there is generally an excess of calcium in surface water and waste-water, calcium concentration does not change appreciably in many wetland treatment systems see Table 11.7.. Bec
Trang 1In addition to the pollutants discussed in earlier chapters,
wastewaters typically contain many other substances Some
of these elements can cause problems when discharged to
receiving waters, and their removal must be considered
dur-ing design These additional materials include salts, acids,
bases, macronutrients, micronutrients, and heavy metals, and
may be categorized in a number of ways Salts include
com-pounds that readily dissociate in water to form charged ions
that may or may not be used as nutrients for plant and animal
growth Common examples of salts are sodium chloride
(NaCl) and gypsum (CaSO4) Acids release a hydrogen ion
when they dissociate (e.g., hydrochloric acid, HCl), and bases
release a hydroxyl ion (e.g., ferric hydroxide—Fe(OH)3)
Spe-cific environmental conditions determine whether the cations
(positively charged ions) and anions (negatively charged ions),
formed when a salt, acid, or base is dissolved in water, are
chemically or biologically active Collectively, ionic
materi-als contribute to the electrical conductivity (EC) of the water
When ionic materials are combined with dissolved nonionic
materials, the result is the total dissolved solids (TDS)
con-tent of the water
Nitrogen and phosphorus, discussed in Chapters 9 and
10, are examples of macronutrients, which have strong
bio-geochemical cycles in a wetland Sulfur also is typically
present in variable but potentially high concentrations, and
has just as powerful influences on wetland functioning The
magnitude of these influences is just emerging as a
control-ling factor on wetland performance for a number of other
pollutants Most obvious is the role of sulfides in
immobiliz-ing trace metals
Iron, aluminum, and manganese are ubiquitous in
wet-lands, but are present at elevated concentrations in mine
drainage waters and the wetlands constructed to treat them
A trace metal can be either a required micronutrient or toxic,
depending on the concentration For example, copper and
zinc are essential elements for plants and animals at low
con-centrations, but they are toxic to some organisms at elevated
concentrations However, for some trace metals, such as
cad-mium and lead, essentiality for plants or animals has never
been found In this chapter, many of the important elements
are discussed, but the list does not include all the elements
that may be found in waters, or all those that might require
treatment The use of a wetland treatment system to modify
the concentration of elements depends on how the elements
interact with the wetland environment and on the wetland
designer’s knowledge of design factors that can enhance or
diminish these processes There is a rapidly growing body
of knowledge about how wetland treatment systems affect
specific trace elements A thorough, updated review of the scientific literature is recommended for project design
A number of substances are considered measures of water quality, but are seldom of concern as pollutants to be treated
in constructed wetlands These include common metals (e.g., sodium, potassium, calcium, and magnesium) as well
as halogens (e.g., fluorine, chlorine, bromine, and iodine) Together with sulfate, these compounds often dominate the total ion content of natural waters and wastewaters In total, they form the major part of EC and TDS Sulfate is of spe-cial importance, because of its active biogeochemical cycle, and interactions with trace metal removal In some treatment wetlands, several of these collective water quality parameters have become important in their own right
11.1 HALOGENS
Chloride and bromide are widely regarded as being vative” in wetland environments, meaning that they interact with the ecosystem to a very limited extent Therefore, they can be used as tracers of water movement in the wetland Usually, chloride is present at concentrations that preclude its use as an injected tracer, but it sometimes serves as a means
“conser-of confirming the wetland water budget Fluoride is usually
a very minor trace constituent in aquatic systems, but there are industrial effluents that contain relatively high concentra-tions The aluminum industry is one such source, including leachates from solid waste disposal sites Bromide is often present at low background concentrations, and injected bro-mide may then be used to trace internal water movements Very little is known about the fate and transport of iodine in freshwater systems
C HLORIDE AND C HLORINE
U.S EPA (2002a, 2006) sets a criteria maximum tion (CMC), which is an estimate of the highest concentration
concentra-of a material in surface water to which an aquatic community can be exposed briefly without resulting in an unacceptable effect The value for chloride is 860 mg/L, and for chlorine
is 19 µg/L U.S EPA (2002a, 2006) also sets a criterion tinuous concentration (CCC), which is an estimate of the highest concentration of a material in surface water to which
con-an aquatic community ccon-an be exposed indefinitely without resulting in an unacceptable effect The CCC value for chlo-ride is 230 mg/L, and for chlorine is 11 µg/L
The chlorine content of wetland plant tissues has not been measured often Results from two projects are shown in
Trang 2404 Treatment Wetlands
Tables 11.1 and 11.2 The Oxnard, California, systems were
exposed to high chloride, and developed high leaf tissue
concentrations (5–40 g/kg dry weight, or 0.5–4.0%)
Presumably, much of the chlorine associated with the dry
matter was originally in solution in the plant water content,
which is 70–80% of the wet weight Therefore sap
concentra-tions would be about five times lower Interestingly,
Salicor-nia spp is a hyperaccumulator of chlorine (Table 11.1) It is
also notable that roots contain much less chlorine than the
shoots Standing dead and litter of Typha latifolia were found
to contain much less chlorine than live leaves at the
Hough-ton Lake, Michigan, treatment wetland (Table 11.2)
Chlorine is biologically interactive in wetland
eco-systems It is influential in the osmolality salinity balance,
but metabolic utilization does not usually cause changes in
water concentrations (Wetzel, 1983) However, there are
cir-cumstances in which utilization can be measured Xu et al.
(2004) measured chloride and sulfate profiles in vertical flow
mesocosms with Typha latifolia in sand, during growth of
the plants The hydraulic loading rate was low (0.66 cm/d),
and consequently, transpiration was an important effect (about 0.3 cm/d) Sulfate was added at concentrations far in excess of any potential plant requirements (80 mg/L SO4-S)
As the water traversed the root zone, sulfate concentrations increased to about double their inlet value, which was strictly attributed to transpiration losses No increase occurred in unvegetated controls However, the profiles of chloride were very different: virtually all of the inlet chloride was absorbed
in the mesocosms, from a starting concentration of about 5.0 mg/L Given the biomass increase of the plants, chloride removal would have produced a chloride content of the cat-tails of about 4,000 mg/kg, which is at the low end of the
range measured for Typha (Tables 11.1 and 11.2).
The more typical situation is an overabundance of ride entering the wetland Because of the relatively low biological demand for chloride, the total chloride mass is usually relatively constant between the inflows and outflows and storages of a treatment wetland (Table 11.3) Therefore, the wetland chloride mass balance can be used to confirm the water budget
chlo-TABLE 11.2
Halogen Content of Biomass Compartments for Typha latifolia in the
Houghton Lake, Michigan, Treatment Wetland in 1991
Note: Units are mg/kg for tissues, and mg/L for water.
Source: Unpublished data.
TABLE 11.1 Chlorine and Fluorine Concentrations in Plant Tissues at Oxnard, California
Note: Units are mg/kg for tissues, and mg/L for water.
Source: Data from CH2M Hill (2005) Additional testing for the Membrane Concentrate Pilot Wetlands Project.
Report to the City of Oxnard Water Division, Oxnard, California, United States.
Trang 3Examples of Conservative Materials Entering and Leaving FWS Treatment Wetlands
HLR (m/yr)
EC In (µS/cm)
EC Out (µS/cm)
Chloride In (mg/L)
Chloride Out (mg/L)
TDS In (mg/L)
TDS Out (mg/L) Pass-Through
Anomalies
New Hanover, North Carolina Full scale 1 0.79 6,256 1,468 2,753 411 5,742
© 2009 by Taylor & Francis Group, LLC
Trang 4406 Treatment Wetlands
Chloride can serve as a tracer of water movement,
espe-cially in the analysis of the very slow underground movement
of water For instance, the progress of a chloride front from
rapid infiltration basins, underground to a monitoring well on
the edge of the receiving wetland, and then out into that
wet-land, is shown in Figure 11.1 The wastewater treatment plant
at Genoa-Oceola, Michigan, received very high chlorides
(about 400–550 mg/L) because of the widespread use of water
softeners in the region The treated water was discharged onto
rapid infiltration basins on a hilltop adjacent to a wetland The
hydrologic gradient moved the water slowly toward the
wet-land, and the high chloride arrived in wells at the wetland edge
after about three years After about six years, the wetland
sur-face waters reflected the chloride of the wastewater, with some
dilution from the other flows in the aquifer
Disinfection: Chlorine in Wetlands
Free chlorine is toxic to most life forms, and is one of the
most frequently used wastewater disinfectants There are
implications for treatment wetlands that receive chlorinated
effluents, because the residual toxicity may negatively
influ-ence the microbial communities within the system
Some of the free chlorine added during disinfection is
converted in solution to chlorides or chloramines, the
lat-ter being regarded as an undesirable pollutant The products
that result from disinfecting water by the addition of chlorine
are:
Free residual chlorine—the portion of chlorine
remaining as molecular chlorine, hypochloride
(HOCl), or hypochlorite ion (OCl –)
Combined residual chlorine—the portion of
chlo-rine that combines with ammonia or nitrogenous
compounds, forming chloramines
Total residual chlorine (TRC)—the sum of free
residual plus the combined residual chlorine
sev-as ammonia Wetlands have enough organic matter to mote formation of trihalomethanes (THM) (Gallard and von Gunten, 2002), but other organic halides may also form Total organic halides (TOX) and halo-acetic acids (HAA)
may also form (Rostad et al., 2000) The photochemical
pro-cess is initiated by production of oxidants such as peroxides These oxidants then oxidize the chlorinated compounds Volatilization, adsorption, and interactions with aquatic plants and the soil system may also contribute to the decay
of residual chlorine
Studies of the loss of TRC were conducted in the Tres Rios, Arizona, FWS wetlands (Wass, Gerke, and Associ-ates, 2004) Disappearance was approximated by first-order behavior The rate constants were calculated to be 0.86 d−1for the Cobble C1 and Hayfield H1 wetlands, based on tran-sect data Thus there would be more than 90% reduction in TRC for a three-day detention time Surveys of organo-chlo-rine compounds in the wetlands showed decreasing gradients from inlet to outlet for TOX, THM, and HAA (Table 11.4)
B ROMIDE AND B ROMINE
Bromide is not commonly measured as a constituent of natural freshwaters or wastewaters It is a common choice for a water movement tracer, and a number of studies have therefore determined the background bromide in treatment wetland waters Example values were 0.2–0.3 mg/L at Tres Rios, Arizona; 0.13–0.18 mg/L at Orlando Easterly, Florida; 0.05–0.15 mg/L at Hillsdale, Michigan; and 0.3–0.4 mg/L
at Des Plaines, Illinois Bromine is, therefore, also found in only minor trace amounts in vegetation Concentrations of
25–46 mg/kg dry mass were measured in Typha latifolia at
the Houghton Lake, Michigan, treatment wetland Parsons
et al (2004) added a uniform sudden dose of bromide to
0 100 200 300 400 500 600
Years of Operation
WWTP Edge well Wetland
FIGURE 11.1 Progress of chloride from the infiltration beds of the wastewater treatment plant (WWTP), underground to a well on the
wetland edge, and then out into the wetland at Genoa-Oceola, Michigan (From unpublished data.)
Trang 5establish an initial surface water concentration of 100 mg/L
in a prairie pothole in Saskatchewan The wetland had no
surface inflow or outflow, and thus the dose remained
con-fined to the system except for infiltration They measured
20–90 mg/kg dry mass in aboveground tissues of Heracleum
lanatum, Polygonum spp., and Carex spp., with localized
values ranging up to 12,700 mg/kg dry mass The fraction of
the dose retained in vegetation was estimated to be 8.7%, as
determined by areal averaging for the diverse species
Bromide sorbs to soils to about the same extent as nitrate
(Clay et al., 2004), which is negligible in most situations
Bromine does not have a role in plant metabolism; however,
bromide can be taken up by plants, to help satisfy the anionic
component of the charge balance in the plant internal water
In that respect, bromide competes with chloride, as
docu-mented by Xu et al (2004) in Typha and Phragmites
sys-tems Plant uptake is, therefore, presumably greatest during
the growing season, during which new plant water is building
within the wetland
F LUORIDE AND F LUORINE
Fluorine in water exists primarily in the form of sodium and calcium salts Calcium fluoride is used as a flux in steel manufacturing Sodium fluoride is used as a drinking water additive for prevention of dental cavities (tooth decay) The recommended optimum level ranges from 0.7 mg/L for warmer climates to 1.2 mg/L for cooler climates Median concentrations are 0.2 mg/L in surface water and 0.1 mg/L
in groundwater (U.S EPA, 2002a) The current Maximum Contaminant Level set by the U.S EPA in 1986 is 4 mg/L Fluoride levels typically range from 0.03 to 0.57 mg/L in
eastern U.K rivers (Neal et al., 2003a).
Fluoride differs from chloride and bromide, because it has been a target of treatment wetland design The aluminum industry relies upon molten salt electrolytes that contain fluo-rides Solid wastes from the industry are usually landfilled, and produce leachates that contain elevated concentrations of fluoride (up to 100 mg/L)
Fluoride partitions more strongly to soils and ments than do bromide and chloride The Langmuir adsorp-tion capacities of soils ranges from 100–400 mg/kg for silts and loams (Bower and Hatcher, 1967) However, the oxyhydroxides of iron and aluminum have much higher bind-ing capacities, 30,000–50,000 mg/kg This property causes
sedi-fluoride to be a poor tracer For instance, LeBlanc et al (1991)
found: “Fluoride was abandoned as a tracer early in the test because fluoride concentrations were rapidly attenuated by
adsorption…” in the mineral soils of the site under study Similarly, Jamieson et al (2002) found only 57% recovery
on a fluoride tracer test of a dairy wastewater treatment land in Nova Scotia
wet-Fluorine is taken up by plants to a moderate extent (see Table 11.1), with tissue concentrations typically in the 100–
500 mg/kg range But because it is not a macronutrient or a micronutrient, it is probable that such uptake is driven by the plant water ionic balance The result of limited uptake and sorption is a limited overall reduction of fluoride in treat-ment wetlands (Table 11.5) Data are too sparse to determine whether seasonal effects are present, or to elucidate possible differences between wetland types or plant varieties
TABLE 11.4
Inputs and Outputs of Chlorination Byproducts in the
Tres Rios, Arizona, Demonstration Wetlands (µg/L)
Example Performances of Treatment Wetlands for Fluorine (mg/L)
Imperial, California Agricultural runoff 0.54 0.56 Unpublished data
Alcoa, Tennessee Aluminum waste leachate 5.80 4.90 Gessner et al (2005)
Russelville, Kentucky Aluminum processing 15.4 8.50 Rowe and Abdel-Magid (1995)
Trang 6408 Treatment Wetlands
11.2 ALKALI METALS
Sodium, potassium, calcium, and magnesium are rarely the
object of regulatory concern, because under most
circum-stances they do not pose any toxicity threat Nevertheless,
each of these has a role in wetland functioning, and can yield
valuable information about pollutant processing and the
wet-land water budget
S ODIUM
Sodium is important in plant and animal physiology Sodium
ions help to regulate osmotic pressure in cells, and therefore
affect the diffusion of all essential growth nutrients between
the external environment and the protoplasm of the living
cells A “sodium pump” fueled by the conversion of
energy-bearing adenosine triphosphate (ATP) maintains internal cell
sodium concentrations at optimal levels The sodium content
of wetland plant aboveground tissues ranges from <0.05% to
more than 1.3% dry weight (Table 11.6) The median across
the 13 species is 0.28%, or 2,800 mg/kg
Because most freshwater wetland species have low
sodium requirements, the dissolved sodium content of
waste-water passing through wetlands changes little (Table 11.7)
Thus, sodium concentrations can be used as a conservative
tracer for calculating dilution and concentration and for
track-ing groundwater discharges from wetlands For instance, the
concentration of sodium in arid land treatment wetlands is
likely to increase during the summer season due to
evapora-tive concentration
Sodium is useful as a marker for added salt (NaCl),
which may enter wastewater treatment systems because of
its use in water softening and road de-icing For example, the
Cumberland County, Pennsylvania, data in Table 11.7, show
a large increase in sodium during a spring flushing event,
which was also accompanied by a large pulse of chloride
(data not shown: Ci = 14 mg/L and Co = 140 mg/L) The gins of the sodium may have been the accumulation of road de-icing salt, contributed by the highway runoff the wetland was designed to treat At the Genoa-Oceola, Michigan, site, discussed in the section on chloride, the water softener salt also had elevated sodium (150 mg/L), compared to the wet-land background of about 5 mg/L The underground plume reached the wetland after about six years, at which time the wetland surface water sodium had increased to 95 mg/L
ori-P OTASSIUM
Ionic pumping maintains potassium levels in plants at centrations of 1.0–4.0% Potassium regulates the open-ing and closing of stomata on plant leaves Stomata are the valves that allow gases inside the plant to be exchanged with the atmosphere Potassium also is used as an enzyme acti-vator in protein synthesis in most cells Potassium typically comprises about 2.6% of the dry weight of wetland plants Potassium concentrations in water of surface flow treatment wetlands are typically between 1.0 and 40 mg/L (Table 11.7), with an average world river concentration of about 3.4 mg/L(Hutchinson, 1975) Potassium has not been the target of treat-ment wetland design In general, there is not much change in potassium from wetland inlet to outlet (Table 11.7)
con-C ALCIUM
Calcium is biologically active because it is used as a ent by invertebrates and vertebrates, and because of its role
nutri-in the carbonate cycle Calcium is required by, and present
in sizeable amounts in, angiosperm plants (Vymazal, 1995) The median concentration in a variety of wetland plants is
TABLE 11.6
Examples of Major Ion Content of Wetland Plants
Plant Type
Sodium (% dw)
Potassium (% dw)
Calcium (% dw)
Magnesium (% dw)
Note: The letter “W” denotes a treatment wetland.
Sources: Data from Boyd (1978) In Freshwater Wetlands: Ecological Processes and Management Potential Academic Press, New York, 155–167; and Vymazal (1995) Algae and Nutrient Cycling in Wetlands CRC Press/Lewis Publishers, Boca Raton, Florida, 1995
Trang 7Examples of Major Cations Entering and Leaving Treatment Wetlands
HLR (m/yr)
In (mg/L)
Out (mg/L)
In (mg/L)
Out (mg/L)
In (mg/L)
Out (mg/L)
In (mg/L)
Hidden River, Florida Urban runoff 2 3.8 0.477 0.828 0.069 0.106 7.08 8.35 0.094
Norco, Louisiana Refinery, West Cell 1 17.8 360 430 8.4 9.1 140.7 46.7 23.4
Cumberland County, Pennsylvania Highway runoff 1 Event — 28.1 62.7 6.54 7.93 16.6 16.2 1.15
Mor˘ina, Czech Republic, HSSF Municipal sewage 1 9.3 127 102 19 20 98 89 21
Slavošovice, Czech Republic, HSSF Municipal sewage 1 9.8 43 16 36 18 41 17 16
© 2009 by Taylor & Francis Group, LLC
Trang 8410 Treatment Wetlands
0.77% dry mass (see Table 11.6), and is similar in fresh-
water planktonic algae However, levels in floating plants
and filamentous green algae range upward to 5–7% dry mass
(see Table 11.6; Vymazal, 1995) The photosynthetic organs
of plants and algae may develop calcium carbonate (calcite)
encrustations in hard water environments Because there is
generally an excess of calcium in surface water and
waste-water, calcium concentration does not change appreciably in
many wetland treatment systems (see Table 11.7)
In some treatment wetlands, there is an iron deficiency,
and calcium biogeochemistry is dominant When this occurs,
the wetland sediments contain a high proportion of calcium
carbonate, which is referred to as calcitic mud or marl The
southern Everglades contain extensive areas of these calcitic
muds, which form under conditions of shorter hydroperiod,
as a result of calcium carbonate precipitation mediated by
periphyton These materials are very dense, low in organic
content, and are typically low in phosphorus content
Calcar-eous periphyton in the south Florida environment contributes
to high soil calcium, with concentrations ranging from 3–4%
in peats to 20–40% in calcitic wetland sediments (Reddy et
al., 1991; DeBusk et al., 2004).
Calcium is also important in constructed wetlands
receiv-ing some types of leachates Municipal landfills may contain
construction materials including gypsum wallboard (calcium
sulfate), and the waste piles from phosphate fertilizer
manu-facture contain mostly calcium sulfate as well
M AGNESIUM
Magnesium is an essential micronutrient because of its role
in phosphate energy transfer and because it is a structural
component in the chlorophyll molecule (Wetzel, 1983)
Because magnesium concentration of surface water almost
always exceeds the requirements for plant growth, elevated
magnesium concentrations are not affected when waste-
water travels through wetland treatment systems
Magne-sium is more soluble than calcium, and precipitate formation
does not occur (see Table 11.7) Plant tissue concentrations
are approximately 0.25% dry weight, but may be higher for
floating plants and filamentous algae (see Table 11.6)
11.3 COLLECTIVE PARAMETERS
H ARDNESS
Hardness measures the concentrations of divalent cations in
a water sample The prevalent divalent ions in most surface
waters are calcium and magnesium Rainwater typically has
low hardness (soft water) with a calcium concentration between
0.1 and 10 mg/L, a magnesium concentration of about 0.1 mg/
L, and a hardness value less than 30 mg/L as CaCO3 Surface
water hardness is variable, depending on the soil and rock
con-centrations of calcium and magnesium, and on the degree of
contact with rocks, soils, and pollution Inland surface water
hardness varies from 10 to 300 mg/L as CaCO3, with a calcium
concentration between 0.3 and 70 mg/L and magnesium centration between 0.4 and 40 mg/L
con-T OTAL I ON C ONTENT
Two chemical parameters are commonly used to indicate the collective concentrations of dissolved substances: TDS and specific conductance These parameters do not specify the distribution of contributing ions and organic compounds that contribute, but they are helpful in support of the wetland water budget Further, the TDS content of water is sometimes
a regulated parameter, especially in arid regions, where salt buildup is a water quality concern
Total Dissolved Solids
TDS is used to quantify the degree of pollution in many industrial wastewater effluents, including textile wastes, food processing wastes, and pulp and paper wastes When dis-charged to surface or groundwaters, these dissolved solids may represent a significant pollution source The total quan-tity of dissolved solids in a water sample is measured by filtration followed by sample evaporation This quantity con-tains both inorganic ions and organic compounds TDS is nearly as conservative in wetlands as specific conductance and chloride Because TDS concentrations are high in many wastewaters and the individual components of these solids greatly exceed the biological requirements for growth, wet-lands generally have a negligible effect on this parameter (see Table 11.3)
Electrical Conductivity
EC, also called specific conductance, of an aqueous tion is the reciprocal of the resistance between two platinum electrodes, 1 cm apart and with a surface area of 1 cm2 The reciprocal of EC is equal to resistance, and is a function of the total quantity of ionized materials in a water sample Specific conductance usually is reported at a temperature of 25°C and in units of µS/cm, or µmhos/cm Measurements can
solu-be made with pocket-portable, inexpensive meters Specific conductance is nearly proportional to the TDS in many sur-face waters and is a convenient measure of the salt content of wastewaters
Total ionic salts in wetlands, as measured by specific conductance, may be somewhat altered by biological con-ditions in wetlands, but physical processes of dilution and evaporation represent the major influences Therefore, EC is
a relatively accurate indicator of dilution and concentration effects by rainfall and runoff and evapotranspiration in wet-land treatment systems
Treatment wetlands are usually, but not always, nated by the introduced flows Rainfall and evapotrans-piration are minor in comparison, except possibly for the duration of extreme events Therefore, in the long run, EC of the inlet and outlet waters are close to the same For the 17 pass-through systems of Table 11.3, the outlet EC averages
Trang 9domi-98% o 2% of the inlet EC This represents long-term mean
performance, over an average of five years Those wetlands
receive an average annual hydraulic loading of 31 m/yr,
which is far greater than precipitation or evapotranspiration,
which is about 1 or 2 m/yr
There are circumstances in which conductivity, chloride,
and TDS change from inlet to outlet, and data then present
a challenge for finding the cause Three such anomalies are
listed in Table 11.3 The first of these is data from the first
17 months of operation of the New Hanover County, North
Carolina, system This FWS wetland treats landfill leachate
that has a high EC (>6,000 µS/cm), and during the start-up
period produced an average outlet EC = 1,468 µS/cm
Chlo-ride and TDS exhibit similar large decreases The reason in
this case is a very low hydraulic loading (0.79 m/yr), coupled
with large rainfall However, the larger effect was the long
time required to replace the low conductivity water used to
initially fill the wetland Both factors produce large dilution
of the incoming leachate
The second illustration is for the Incline Village, Nevada,
wetland This arid-climate system does not receive water in
the summer, because it is used to irrigate fodder crops The
design of the wetland was for disposal, primarily (y90%) to
evaporative losses, and secondarily (y10%) to infiltration
The hydraulic loading is very small, and large
concentra-tion increases in chloride and TDS are produced as the water
moves through the sequence of cells (Kadlec et al., 1990).
The third illustration is the Ouray, Colorado, wetland,
which exhibits twofold increases in TDS over a five-year
averaging period (HDR/ERO, 2001) This is a strong signal
of secondary sources of water entering the treatment
wet-land This has been identified as a maintenance issue: “The
wetland system experiences an outside flow problem with
sulfates, which concentrate.…”
Conductivity has also been used as a diagnostic tool
for internal processes in treatment wetlands in a number
of ways For example, EC is often much higher in the pore
waters of FWS wetland soils and sediments than it is in
over-lying waters DBE (2003) measured the EC of surface waters
and pore waters in Cell 1 of the ENRP in 2001 The pore water EC was higher than that of the overlying surface waters (Table 11.8) Among the potential reasons is that rooted plants extract their transpiration requirement from pore water, but reject some or all of the associated salts The result
is an upward positive gradient in EC in the top soil layer That gradient may continue into the overlying water, and pro-duce stratification of the EC of the water column The pattern
of these results indicates an internal recycle loop, in which dissolved substances are drawn down into the root zone by transpiration or other flows, only to be rejected by the plants
to avoid buildup of TDS within their tissues This creates an upward gradient, which causes diffusive solute movements back into the water column from the pore water
Density-Induced Vertical Stratification
Conductivity is also a tool to understand the phenomenon
of density stratification in constructed and other wetlands Wetlands are typically too shallow to stratify due to thermal gradients, but the same is not true for density segregation, which may exist due to the character of incoming wastewater, rainfall, or added tracers Two examples will serve to illus-trate the potential for vertical stratification
Salt Plumes in FWS Wetlands
Various salts, such as sodium bromide and lithium chloride, are convenient tracers for water movement Considerable quantities are needed, and consequently it is tempting to add concentrated solutions, in order to deal with manageable tracer solution volumes for addition However, when dense solutions are introduced into the bottom of wetlands, there may be a strong energy barrier to vertical mixing, resulting
in the dense material remaining on the bottom of the wetland Concentrations used in a South Florida Water Management District (SFWMD, 2002) tracer study were 7.5% LiCl (density
= 1.04 g/cm3) (Söhnel and Novotny, 1985) Concentrations of sodium bromide in a Tres Rios, Arizona (Whitmer, 1998), tracer study were about 20% NaBr (density = 1.16 g/cm3)
TABLE 11.8
Pore Water Concentrations of Alkalinity, Calcium, and Electrical Conductivity in Cell 1 of the
ENRP Wetland in Florida
Note: EAV = emergent aquatic vegetation; SAV = submerged aquatic vegetation; FAV = floating aquatic vegetation.
Source: Data from DBE (2003) Assessment of hydraulic and ecological factors influencing phosphorus removal in Stormwater
Treat-ment Area 1 West Final report to Florida DepartTreat-ment of EnvironTreat-mental Protection, Contract No WM795, April 2003.
Trang 10412 Treatment Wetlands
(Söhnel and Novotny, 1985) It is noteworthy that
demonstra-tion of stratificademonstra-tion in limnology laboratory courses utilizes
densities of 1.105 and 1.05 g/cm3 (Wetzel and Likens, 1991)
More directly, the work of Schmid et al (2003, 2004b) shows
that both tracer injections would lead to stable, unmixed layers
of tracer on the wetland bottom Both tracer studies showed
very poor tracer recovery, suggesting that the tracer “got
stuck” in the wetland sediments
Further evidence of vertical stratification was reported
by Chimney et al (2006), for a constructed wetland in the
Florida Everglades (Figure 11.2) In this case, a likely cause
is the back-diffusion of salts from the concentrated pore
water, as described in Table 11.8
Stratification in HSSF Wetlands
The presence of a gravel matrix in a HSSF wetland serves to
exacerbate the potential for vertical stratification It is well
known that flows through clean porous media are
suscep-tible to layering For example, Wood et al (2004) found that
density effects occurred when the invading solution tration was greater than approximately 13,000 mg/L It is not
concen-surprising that Drizo et al (2000) found that tracer bromide
at 20,000 mg/L sank to the bottom of HSSF wetlands Rash and Liehr (1999) have also reported stratification effects in HSSF wetlands
The Grand Lake, Minnesota, wetland exhibited large vertical stratification during a start-up period of two years, as evidenced by much higher EC in the bottom water samples
than in the top samples (Figure 11.3; Kadlec et al., 2003)
These wetlands were initially filled with water from an cent natural bog, which had lower EC than the incoming wastewater The stratification persisted, as a result of the very low flow over the summer and fall of 1996 The stratifica-tion was mitigated in the fall of 1996 by pumping bottom water to the surface, although it restratified the next spring but not as strongly After about two years of operation, only mild stratification existed, with 21% higher EC in the bottom water samples than in the top samples
adja-–70 –60 –50 –40 –30 –20 –10 0
Conductivity (µS/cm)
Emergent SAV
FIGURE 11.2 Vertical stratification of electrical conductivity in the ENRP, Florida constructed FWS wetland Points represent the averages
for 141 dates during May 1995 to October 1997 (Data from Chimney et al (2006) Ecological Engineering 27(4): 322–330.)
0 500 1,000 1,500 2,000 2,500 3,000 3,500 4,000
Days
Inflow Outflow Top Bottom
FIGURE 11.3 Electrical conductivity for Grand Lake, Minnesota, HSSF wetland cell #1 Introduction and removal were at the cell bottom
High conductivity water persisted at 45 cm depth for about two years, and low conductivity water persisted at 15 cm depth The influence of
snow melt can be seen in the lower conductivity values on the top in each early spring (Adapted from Kadlec et al (2003) In Constructed
Wet-lands for Wastewater Treatment in Cold Climates Mander and Jenssen (Eds.), WIT Press, Southampton, United Kingdom, pp 19–52.)
Trang 1111.4 SULFUR
Sources of sulfur include geochemical weathering of
miner-als, wind-blown sea salt, and emissions from fossil-fuel
com-bustion (Wetzel, 1983) Large quantities of sulfur enter the
atmosphere from natural and industrial sources, and return to
earth as acid precipitation containing sulfates (sulfuric acid)
Treatment wetlands receive these atmospheric inputs as well
as sulfur compounds that may be included in the chemicals in
the water to be treated Municipal wastewater contains sulfur
compounds, originating from the potable water supply, and
augmented by waste products Drinking water standards are
strict for sulfide (2 µg/L), but less so for sulfate (250 mg/L)
Hydrogen sulfide is a reactive and toxic gas with problematic
side effects, including a rotten egg odor, corrosion, and acute
toxicity
The processing of sulfur in wetland ecosystems is
rep-resented by interconversions of several sulfur compounds in
the different micro-regions of the ecosystem (Figure 11.4)
Oxidized forms, such as sulfite, sulfate, and thiosulfate, are
found in the oxygenated portion of the FWS water column
Reduced forms, including sulfide, bisulfide, and elemental
sulfur, are found in the soils and sediments under conditions
of low redox potential Ionic and molecular forms are
preva-lent Hydrogen sulfide and methylated sulfur compounds are
volatile, and may be lost from the wetland to the atmosphere
Sulfate is an essential nutrient because its reduced, sulfhydryl
(-SH) form is used in the formation of amino acids Because
there is usually enough sulfate in surface waters to meet the sulfur requirement, sulfate rarely limits overall productivity
in wetland systems
Although seldom a water quality target in its own right, sulfur is an important part of the chemical processing in wet-lands From a treatment perspective, sulfur has a critical role
in the formation and storage of metal sulfides In this tion, the principal reactions of sulfur in the environment are explored, together with the treatment and storage potential.Sulfur concentrations in wetland plant tissues typically range from 0.1–0.6% dry mass, but algal concentrations may
sec-be considerably larger (Table 11.9) Belowground tissues have not often been measured, but are considerably higher than aboveground plant part concentrations Treatment wet-land sediments contain sulfur at 0.1–1.0% dry mass
D ISSIMILATORY S ULFATE R EDUCTION
Aerobic organisms excrete sulfur as sulfate However, upon death and sedimentation, heterotrophic bacteria release the sulfur in the reduced state, which can result in the accumu-lation of high levels of hydrogen sulfide in wetland sedi-ments A second process that transforms sulfate and other oxidized sulfur forms (sulfite, thiosulfate, and elemental sulfur) to hydrogen sulfide in anaerobic sediments, dissimi-latory sulfate reduction, is mediated by anaerobic, heterotro-
phic bacteria such as Desulfovibrio and Desulfotomaculum, which use sulfate as a hydrogen acceptor (Castro et al., 2002;
Aerobic Soil Layer
FIGURE 11.4 Sulfur pathways and forms in FWS wetlands (From Mitsch and Gosselink (1993), Wetlands Second Edition, Van Nostrand
Reinhold Company, New York Reprinted with permission.)
Trang 12414 Treatment Wetlands
Lloyd et al., 2004) The presence of decaying organic matter
in the wetland sediments and soils depletes oxygen and
cre-ates acid pore waters Organic matter fuels sulfate reduction
Equation 11.1 is favored at low pH, while Equation 11.2
dominates at higher pH As ferrous sulfide (FeS) is highly
insoluble, hydrogen sulfide does not tend to accumulate
until the reduced iron is removed from solution When ion
concentrations are low, or when sulfate and organic matter
concentrations are high, significant hydrogen sulfide
concen-trations can occur Several other metal sulfides are also very
insoluble, including ZnS, CdS, and others
Sulfate is mildly sorbable on soils For example, Fumoto
and Sverdrup (2001) found Freundlich isotherm parameters
of 0.17 < KF < 0.44 [units: (mol/kg) × (mol/L)–n ] and n = 0.078
for mineral soils For water at 20 mg/L, the resultant sorbed amounts were measured in the range 250–500 mg S/kg
H YDROGEN S ULFIDE
Hydrogen sulfide exists in water solution as un-ionized (H2S)
or singly or doubly ionized (bisulfide, HS−, or sulfide, S2−), depending on water temperature and pH The two dissocia-tion reactions are:
Above (mg/kg)
Below
Plants
Sediments
30–50 cm (11 lakes, Poland) 16–227 — 80–2,890 Samecka-Cymerman and Kempers (2001)
Note: Water concentration (mg/L) is for sulfate.
Trang 13C oonized hydrogen sulfide concentration, mol//L
first dissociation constant, dimensio
At equilibrium, the un-ionized form is predominant at low
pH, and bisulfide is dominant at high pH in aqueous systems
(Figure 11.5) However, equilibrium is not necessarily attained
in wetland systems, because of continual influxes of sulfate,
and a large number of microbially mediated processes that
may occur In the presence of sulfate in aqueous solution,
oxi-dation prevails at Eh > −300 mV at circumneutral pH (Pankow,
1991) In wetlands, the sulfate reduction zone occupies the
range −200 < Eh < −100 mV (Reddy and D’Angelo, 1994)
Nonetheless, there may be large fractions of un-ionized H2S,
which is volatile and may be lost to the atmosphere
Volatilization of hydrogen sulfide requires mass transport
to the air–water interface, followed by transfer into the air,
and follows rules analogous to those discussed for ammonia
volatilization (see Chapter 9) The Henry’s law constant for
H2S at 25°C is 3.49 mg/L·atm, which indicates large volatility
At other temperatures, the Henry’s law constant, in units of
mol fractions in the liquid and gas, is given by Lide (1992):
¤
¦¥
³µ´
environ-Hydrogen Sulfide in Municipal Wastewater Treatment Wetlands
The Listowel, Ontario, system studied five wetlands for four years, including the H2S content of the incoming and outgoing waters (Table 11.10) (Herskowitz, 1986) The sulfate content was only infrequently monitored, but was typically in the range of 170–200 mg/L Alum additions to wetlands 1, 2, and 3 accounted for 24 mg/L of the incoming sulfate There were marked differences between wetlands of high aspect ratio (Systems 1, 3, and 4), which had lower outlet H2S, and those of low aspect ratio (Systems 2 and 5), which had much higher outlet H2S All systems produced hydrogen sulfide in the warm months
As a point of reference, the rate of emission of H2S was measured in anaerobic ponds in the Mediterranean climate at
Meze, France (Paing et al., 2003) The pond reduced sulfate
0 20 40 60 80 100
pH
Molecular H2S Bisulfide Sulfide
FIGURE 11.5 Aqueous equilibrium concentrations of sulfide and bisulfide at 25°C Based on dissociation constants from Lange’s
Hand-book of Chemistry (1985).
TABLE 11.10 Hydrogen Sulfide in the Listowel, Ontario, Constructed Wetlands, 1980–1984, in mg/L
Trang 14416 Treatment Wetlands
from 165 mg/L to 57 mg S/L, but produced sulfides, with an
increase from 3.8 to 19.2 mg S/L The H2S emission rates were
found in the range of 20–576 mg S/m2·d (mean = 172) This led
to atmospheric concentrations as high as 5 ppm, which is well
above the human odor threshold of about 0.05 ppm Almasi
and Pescod (1996) also found high sulfides in ponds for warm
(25°C) and cool (10°C) conditions, in the range 15–60 mg/L,
leading to H2S concentrations of 2–12 mg S/L
O XIDATION OF S ULFUR AND S ULFIDES
When it is exposed to air or oxygenated water, hydrogen
fide may be oxidized back to sulfate This may occur via
sul-fur bacteria such as Beggiatoa, which promotes the oxidation
of hydrogen sulfide to elemental sulfur:
Photosynthetic bacteria, such as purple sulfur bacteria, use
hydrogen sulfide as an oxygen acceptor in the reduction of
carbon dioxide, resulting in partial or complete oxidation
back to sulfate:
where CH2O represents organic matter
Under some circumstances, treatment wetlands have
been observed to turn purple, as happened in a FWS
treat-ing high-strength potato processtreat-ing wastewater (P Burgoon,
personal communication)
In any case, these microbially mediated reactions suggest
that elemental sulfur may be found in treatment wetlands
Anecdotal reports of elemental sulfur have been made for the
Houghton Lake, Michigan, system; the Tres Rios, Arizona,
wetlands; the Brighton, Ontario, system; and the Nucˇice,
Czech Republic, HSSF system In extreme situations, a
whit-ish colloid or adhering whitwhit-ish precipitate is seen in the
out-flow from the treatment wetland (Figure 11.6)
Gammons et al (2000a) comment about this
phenom-enon in connection with the Butte, Montana, mine drainage
treatment wetlands:
cells created a foul smell and also resulted in unsightly
pre-cipitates of colloidal sulfur in downstream aerobic waters It
is evident from the above observations that optimal wetlands
performance is in some respects a delicate balancing act
Too much BSR [biological sulfate reduction] activity results
in an undesirable accumulation and release of H 2 S, whereas
too little results in decreased metal attenuation.
Winter and Kickuth (1989b) reported about 36% of the removed sulfur in a HSSF wetland treating textile industry wastewater was stored in the form of elemental sulfur
O RGANIC S ULFUR
Organic sulfur compounds account for a good share of the sulfur found in wetland sediments For instance, 84–88%
of the total sulfur in a New Jersey peat was organic sulfur
(Spratt et al., 1987), and over 90% in a West Virginia peat
(Wieder and Lang, 1988) In treatment wetlands, the storage
of sulfur is also in major part associated with humic als For instance, Winter and Kickuth (1989b) reported about 30% of the removed sulfur was in humic materials
materi-Additionally, there are several low molecular weight organic sulfur compounds that may be found in wastewater Methanethiol (CH3SH) and dimethyl sulfide (DMS or (CH3)2S) are perhaps the most common, and are quite volatile (Faulkner
and Richardson, 1989; Lomans et al., 2002) Both are extremely
odiferous There are several mechanisms that can produce and destroy these volatile organic sulfur compounds (see Lomans
et al., 2002) Kiene and Hines (1995) found both were formed
in natural fen peat at the same rate of 40 nmol/L·d (256 µg/m2·d
in the top 20 cm of soil) Wood et al (2000) measured DMS
removals of 80% (152–28 mg/L) in SSF wetlands treating swine wastewater, and attributed the loss to mineralization and oxidation Domestic wastewater contains lesser amounts
of DMS, and reductions are not significant for anoxic HSSF
systems Huang et al (2005b) found small removals,
averag-ing 20% (2.24 µg/L down to 1.79 µg/L) Their studies involved eight wetlands, with average redox of −35 mV, and reductions
of sulfate of 60% (72.5 mg/L down to 29.4 mg/L)
P HYTOTOXICITY
Lamers (1998) documents that sulfate has negative effects on
the growth rate of Carex nigra, Juncus acutiflorus, and Gallium
FIGURE 11.6 (A color version of this figure follows page 550)
This HSSF wetland outlet structure at Tamarack, Minnesota, has become coated with elemental sulfur.
Trang 15palustre, at concentrations of 64 and 128 mg S/L Koch and
Mendelssohn (1989) report that 32 mg S/L of sulfide produced
negative effects in Panicum hemitomon and Spartina
alterni-flora The presence of sulfide is coupled with anaerobic
con-ditions in the root zone, but the effects of sulfide go beyond
mere anoxia (Koch et al., 1990) Hydrogen sulfide apparently
inhibits the activity of alcohol dehydrogenase, thereby limiting
the ability of plants to avail themselves of alternative anoxic
energy pathways This effect was confirmed by measuring a
reduced 15N uptake rate in the presence of sulfide However,
the availability of free sulfide is strongly mediated by the
pres-ence of iron, because of the formation of iron sulfides
Phytotoxicity was found to be very serious at the 45-mg
S/L level in Phragmites australis (Armstrong et al., 1996)
These authors found that aeration pathways became blocked,
interfering with the diffusive connection to the atmosphere,
and thus reducing the plant’s ability to oxygenate the
rhi-zosphere Smolders and Roelofs (1996) found for Stratiotes
aloides, an aquatic macrophyte characteristic for
mesotro-phic freshwater marshes, that levels of 320 mg S/L were toxic
to the roots) Lamers et al (2002) found root parts, growing
in 1.7–3.4 mg S/L of sulfate into the peaty sediment, clearly
showed sulfide toxicity by becoming black, slimy, and unfit
for nutrient uptake from the sediment Free sulfide could not
be detected in the surface water They concluded that only
roots in the surface water would survive Nuphar lutea did
not propagate in the sulfate-treated enclosures However, the
sensitivity of a wetland plant species to free sulfide not only
depends on the actual sulfide levels in the rhizosphere, but
also on detoxification mechanisms like radial oxygen loss
As noted above, high sulfide concentrations in freshwater
sediments may also lead to higher fluxes of volatile organic
sulfur compounds to the atmosphere due to the microbial
methylation of hydrogen sulfide
P ERFORMANCE OF W ETLANDS FOR S ULFUR R EMOVAL
Since sulfate inputs in surface flow wetland treatment systems
frequently exceed the biological requirements of wetland
biota, wetlands generally are not as effective for removal of
sulfur as for other contaminants (Wieder, 1989) Although
microbial routes provide for gaseous losses of H2S and DMS,
these require the very low redox potentials usually found
only in deeper wetland sediments Metal sulfide precipitation
often blocks much of the gaseous loss by immobilizing
sul-fides in the sediments Plant storage is minimal, for instance
plant uptake was estimated at 1.5 g S/m2·yr in a natural bog
(Hemond, 1980) Winter and Kickuth (1989a,b) reported only
1% taken up by plants in a HSSF treatment wetland
Conse-quently, the majority of sulfur removal will generally be to
organic, elemental, and metal sulfide forms in the wetland
sediments
As a result, the median-observed concentration
reduc-tion is only 14% for 32 wetlands (Table 11.11) Only a few
mine water wetlands show more than 50% reduction, and
that may be attributed to the anaerobic mode of operation
in some cases Subsurface horizontal flow wetlands also
sometimes satisfy this anoxic condition Winter and Kickuth (1989a, b) reported that a root-zone, soil-based treatment sys-tem receiving textile wastewaters from a facility in Bielefeld, West Germany, removed from 80–85% of the sulfur mass at
an hydraulic loading rate of 1.14 cm/d for a removal rate of 9.6 kg/ha·d These authors reported that the majority of this sulfur was largely stored in the wetland soil as elemental sul-fur (31%) and organic sulfur (25%), and that only a small fraction was released by volatilization to the atmosphere
Huang et al (2005b) observed 24–88% reduction for
hydrau-lic loadings of 2.0–4.5 cm/d, corresponding to fur loadings of 5–10 kg/ha·d In Table 11.11, results from five HSSF constructed wetlands in the Czech Republic are pre-sented The median removal is 51%, indicating anaerobic conditions in the beds with horizontal sub-surface flow How-ever, Vymazal and Kröpfelová (2006) pointed out that despite removal of sulfates, elimination of ammonia may occur at the same time The question remains to be answered whether this removal is due to “conventional” aerobic nitrification, which may proceed in aerobic microzones adjacent to plant roots, or due to Anammox, i.e., anaerobic ammonia oxidation
sulfate–sul-Sulfate removal should not be viewed as a process that
is independent of other wetland chemistry and processes
For instance, studies by Wiessner et al (2005a) determined
that sulfate reduction was strongly dependent on ter biochemical oxygen demand (BOD), presumably acting
wastewa-as a carbon source, in a manner analogous to tion BOD of 200 mg/L led to 100% removal of sulfate Conversely, ammonia reduction decreased from 75 to 25%
denitrifica-as sulfate reduction incredenitrifica-ased Wiessner et al (2005b)
conclude that the importance of the sulfur transformation processes inside the rhizosphere of constructed wetlands, even in the case of treatment of domestic wastewater, has been underestimated Extreme variations of removal pro-cesses in large-scale treatment wetlands may reflect this fact The sensitivity of nitrification, for example, could be due to nutrient or oxygen limitations, but could also have been additionally or exclusively caused by products of sul-
fur transformation Wiessner et al (2005b) suggest that, in
view of the interesting high application potential of simple wetland systems for the removal of metals by sulfide pre-cipitation or the treatment of sulfate-rich wastewaters such
as acid mine drainage, the dynamics of the sulfur cycle in the rhizosphere should be understood in more detail
S ULFUR -I NDUCED E UTROPHICATION
Interactions also may exist between sulfur processing and phosphorus removal in treatment wetlands In some systems, but not all, a fraction of the accreted phosphorus is bound
by iron-containing substances Other fractions are bound in calcium-rich materials, or in organic components of soils and sediments Two effects have been reported: (1) a reduction
of phosphorus uptake due to sulfide toxicity, and (2) sulfide binds iron and interferes with that component of phosphorus storage that relies upon the iron–phosphorus link (Lamers
et al., 1998).
Trang 16418 Treatment Wetlands
The response of wetlands to new sources of sulfate,
and ultimately sulfide in the sediments, therefore, differs
considerably depending upon the sources and quantities
of iron in the wetland (Lamers et al., 2002) For
exam-ple, a Typha-Carex wetland at Tienhoven near Utrecht,
Netherlands, had relatively high iron, and a continuing
sup-ply from groundwater Addition of sulfate caused oxidation
of iron in response to sulfate reduction, and considerable quantities of phosphorus were released However, a second
wetland, dominated by Nuphar surrounded by Phragmites,
in Weerribben National Park, Netherlands, did not have a groundwater supply of iron Sulfate additions to that wet-land caused large quantities of sulfide formation, but no phosphorus was released
TABLE 11.11
Example Performances of Treatment Wetlands for Sulfate Reduction
Inlet (mg/L)
Outlet (mg/L)
Reduction
Mine Water
Northumberland, United Kingdom Shilbottle 1 8,000 2,000 75 Batty and Younger (2004)
Leachate
Agricultural Runoff
Industrial
Municipal Wastewater
Municipal HSSF
Trang 1711.5 TRACE METALS: GENERAL
CONSIDERATIONS
T OXIC E FFECTS IN W ATER AND S EDIMENTS
A number of trace metals are essential micronutrients at low
concentrations, but some trace metals may occur in municipal
wastewaters at concentrations that are toxic to sensitive
organ-isms The probability of exceeding sensitive toxicity levels
in mine water, leachates and some industrial waters is much
higher For most trace elements, biochemical transformations
and chemical characteristics can lead to biomagnification, a
phenomenon in which increasing concentrations occur in
con-sumers along a food chain Although most trace metals are
more concentrated in biological tissues and soils than they are
in surface water, hazardous situations do not always occur
Metals in wastewater must be removed prior to final
dis-charge to protect the environment from toxic effects, but the
use of wetlands to accomplish this goal must be examined
cautiously Surface flow wetland treatment systems are open
to biota that may be exposed to potentially dangerous levels
of metals, primarily in the wetland sediments The removal
of metals can result in storage in sediments that is inimical
to the subset of wetland organisms that live or feed in those
sediments To prevent this problem from occurring, wetland
treatment system designers and regulators should consider
pretreatment to reduce influent metal concentrations Deep
water systems with floating plants send sediments to depths
that are out of reach of top feeders A second alternative is to
minimize the opportunity for ingestion of metals Subsurface
flow wetlands accomplish this purpose
In the United States, most treatment wetlands are not
con-sidered waters of the United States, and would therefore not
be required to meet water quality guidelines for the waters they are designed to protect The levels of metals that may be tolerated by sensitive organisms have been promulgated in the form of guidelines for the protection of receiving waters and associated sediments Examples of such guidelines are presented in Tables 11.12 and 11.13 These may or may not
be considered applicable to treatment wetlands, which are not necessarily themselves protected by U.S water quality guidelines
A BIOTIC M ETAL P ARTITIONING
Depositing sediments are capable of adsorbing significant quantities of trace metals directly or indirectly through the accumulation of coatings such as organic matter, iron, and manganese oxyhydroxides, which will in turn act as trace ele-ment collectors Organic matter, which may exist as a sur-face coating or as a particulate, may play an important role
in metal speciation and bioavailability Microbial position of organic matter typically results in sediments that are anoxic under a thin oxic surface layer Under these anoxic conditions, divalent cationic metals such as cadmium, copper, lead, nickel, and zinc are readily form metal sulfides
decom-As long as amorphous sulfide concentrations are in excess of the total trace-metal concentration (on a molar basis), these metals will occur predominantly as insoluble metal sulfides
In anoxic sediments, metals in excess of sulfide may complex with organic matter This buffers organisms against metal toxicity (Doig and Liber, 2006)
An appreciation of transformation rates of divalent ionic partitioning is needed to predict behavior and risk within natural environments Although divalent cationic metals are not redox-active species within soil or aquatic environments,
U.S EPA Human Health (µg/L)
Note: As noted, some are hardness-dependent The criteria maximum concentration (CMC) is an estimate of the highest concentration of a material in
surface water to which an aquatic community can be exposed briefly without resulting in an unacceptable effect The criterion continuous concentration (CCC) is an estimate of the highest concentration of a material in surface water to which an aquatic community can be exposed indefinitely without resulting in an unacceptable effect U.S EPA numbers are provided in U.S EPA (2002a, 2006) Screening quick reference tables (SQRT) are provided
by National Oceanic and Atmospheric Administration (1999).
Trang 18420 Treatment Wetlands
oxidation and reduction reactions may nevertheless affect
partitioning Retention can be modified by changes in
sub-strate chemistry For instance, zinc sorbs strongly to iron and
manganese oxyhydroxides in aerated systems, and reacts with
hydrogen sulfide to yield zinc sulfide in anaerobic
environ-ments Thus, changes in redox status may shift zinc
partition-ing For example, reductive dissolution of iron and manganese
oxyhydroxides under anaerobic conditions releases zinc into the
aqueous phase; persistence of anoxic conditions may then lead
to a repartitioning of zinc into sulfide or carbonate precipitates
However, slow transformation rates and fluctuation in
condi-tions may alter these predicted phase changes Redox is affected
by wetland water depth, and depth is therefore a partial
surro-gate for redox At a contaminated wetland site in Idaho, these
speciation effects were observed (Table 11.14) (Bostick et al.,
2001) There are associated consequences for metal removal
For instance, for zinc, an increase in water depth from 0.3 to
1.0 m produced a decrease in removal from 38–18% for a fixed
detention time of one day (Gillespie et al., 2000).
where
a C
Langmuir parameter, L/mgmetal concentr
metal concentraS
Langmuir parameter
The maximum capacity for metal is CSmax = K/a, which
is only achieved at high water concentrations The
half-satu-ration water concenthalf-satu-ration, where C S = 0.5CSmax, is equal to
1/a At low water concentrations, CL << 1/a, the Langmuir
relation reduces to a linear partition equation:
Lesage et al (2006) reported that removal of Co, Ni, Cu,
and Zn by gravel and straw could be well described by the Langmuir isotherm with R2q 0.97 for gravel and R2q 0.93 for straw El-Gendy (2006) reported that sorption of heavy
TABLE 11.13
Guidelines for Metal Concentrations in Sediments
Wisconsin TEC (µg/g) PEC (µg/g)
Background Level (mg/L)
Lowest Effect Level (µg/g)
Severe Effect Level (µg/g) SQRT (µg/g)
Note: Wisconsin (WDNR, 2003) levels are a threshold effect concentration (TEC) and a probable effect concentration (PEC)
Ontario guidelines from OMOEE (1994) Screening quick reference tables (SQRT) are provided by National Oceanic and
Atmos-pheric Administration (1999).
TABLE 11.14
Speciation of Sedimentary Zinc as a Function of
Water Depth in a Metal-Contaminated Wetland
Water
Depth (cm)
ZnO (%)
Hydroxide-Sorbed Zn (%)
ZnS (%)
ZnCO3 (%)
Note: Values are for the top 5 cm of sediment cores.
Source: Adapted from Bostick et al (2001) Environmental Science
and Technology 35: 3823–3829.
Trang 19metals from the landfill leachate by roots of water hyacinth
(Eichhornia crassipes) could be described by both
Lang-muir and Freundlich isoterms with respective correlation
coefficients R2 of 0.94 and 0.93 Organic sediments contain
polar functional groups such as acids and phenolics that are
responsible for cation exchange capacity (CEC), and can be
involved in chemical binding (Ho and McKay, 2000) The
metal-sediment reaction may be represented as:
2
where P represents the organic material (peat).
If Equation 11.14, cation exchange, is presumed to
repre-sent data, then the amount of metal bound is reprerepre-sented by
(Kadlec and Keoleian, 1986):
eq
HH
where the bracket notation denotes molar concentration This
suggests that the partition coefficient ([MP2]/[M2+] = CS/CL =
K) should go down markedly with decreasing pH, which is
in fact the observation of many investigators, as shown in
Kadlec and Keoleian (1986)
E QUILIBRIUM M ETAL C HEMISTRY C ALCULATIONS
There are several computer codes that have been developed to
compute the theoretical thermodynamic equilibria in water
solu-tions For instance, MINTEQA2 is an equilibrium speciation
model that can be used to calculate the equilibrium composition
of dilute aqueous solutions in the laboratory or in natural
aque-ous systems (U.S EPA, 1991) The model calculates the
equi-librium mass distribution among dissolved species, adsorbed
species, and multiple solid phases under a variety of
condi-tions A comprehensive database is included that is adequate for
solving a broad range of problems without need for additional
user-supplied equilibrium constants The model employs a
pre-defined set of components that includes free ions and neutral
and charged complexes The database of reactions is written in
terms of these components as reactants An ancillary program,
PRODEFA2, serves as an interactive preprocessor to help
pro-duce the required MINTEQA2 input files Code to achieve
sim-ilar results, PHREEQC, is available from the U.S Geological
Survey (Parkhurst et al., 1980) These equilibrium calculations
may be used to prepare solubility diagrams for metals in the
presence of a variety of anions (see, e.g., Figure 11.7)
There are, however, substantive discrepancies that occur
between predictions and observed wetland water chemistry
Solubility calculations for a mesocosm of homogenized
sedi-ment indicated supersaturation with respect to the sulfides
of iron, copper, nickel, and zinc, yet measurements
demon-strated a substantial supply of both trace metals and sulfide
from the solid phase to the pore waters (Naylor et al., 2005)
Ratios of metals measured in pore waters were consistent with
their release from iron and manganese oxides, indicating that
supply, as much as removal processes, determines the
pseudo-steady state concentrations in the pore waters The Naylor et al
(2005) observations suggest that trace metals are not ately bound in an insoluble, inert form when they are in con-tact with sulfide As a result of the complex wetland situation, forecasts from computer programs such as MINTEQA2 are not accurate representations of wetland situations For exam-ple, Frandsen and Gammons (2000) found predictions of zinc remaining in solution to be underestimated by several factors
immedi-of ten at low water concentrations, and to be strongly dent upon the assumed form of the solid sulfide (Figure 11.8).The reasons for such large discrepancies are presumably related to the complexities of the treatment wetland envi-ronment, compared to abiotic laboratory experiments with controlled water chemistry The calculations are for thermo-dynamic equilibrium conditions, which may not be satisfied for the dynamic conditions of flow through wetlands Unfor-tunately, it would appear that equilibrium calculations are of little value in predicting treatment wetland performance for metal removal
depen-D ESIGN E QUATIONS FOR M ETAL R EMOVAL
The literature does not currently contain a clear indication of what first-level design calculation should be used for treat-ment wetland sizing for metal removal The two simplest choices are a fixed load removal or a first-order areal calcula-tion The former is advocated in the mine water treatment
literature (Hedin et al., 1994; Younger, 2000; Younger et al.,
2002), and is termed the area-adjusted contaminant removal rate This is essentially a zero-order model, which fixes the removal rate per unit area of the wetland:
–400 –200
–600
PbS PbCO3PbSO4
FIGURE 11.7 Solid phases of lead in the presence of sulfate, sulfide,
and carbonate (From DeVolder et al (2003) Journal of
Environ-mental Quality, 32(3): 851–864 Reprinted with permission.)
Trang 20Tarutis et al (1999) determined RA values for 35
wet-lands for iron and manganese, and found median and mean
values of 3.5 and 6.5 g/m2·d for iron and 0.24 and 0.73 g/m2·d
for manganese, respectively Younger et al (2002) found RA
median and mean values of 10 and 11.4 g/m2·d for iron (N =
20 wetlands) and 0.10 and 0.28 g/m2·d for manganese (N = 17
wetlands), respectively However, in both studies, the
coef-ficients of variation were unacceptably large, in the range of
100–200% This zero-order uptake model would correspond
to a fixed rate of supply of a precipitating reactant, such as
sulfide The subsequent sections of this chapter show that
metal removal is not constant for most wetlands, but strongly
correlated to the metal loading to the wetland
The second choice, a first-order model, presumes that
more detention time (lower hydraulic loading) will result in
greater metal removal, and that higher inlet concentrations
will result in more removal It is consistent with the concept
of mass transfer of the metal to the reactive sediment layer,
which is driven by the concentration difference between
water and sediment pore-water metals Younger states that
“However, as the design of passive systems advances, it is
likely that volume-based or retention-time based measures
of performance will prove to be more appropriate in many
circumstances.” Tarutis et al (1999) concluded that evidence
showed that the first-order model was a better choice, and
advocated the plug-flow form:
C C
kA Q
where
k areal rate constant, m/d
Data from 35 wetlands gave a mean value k = 0.29 m/d (106 m/yr) for iron, and k = 0.057 m/d (21 m/yr) for manga- nese (Tarutis et al., 1999) Younger et al (2002) reported k = 0.105 m/d (38 m/yr) for iron, and k = 0.061 m/d (22 m/yr) for
manganese, at the Quaking House system
Goulet et al (2001) examined the efficacy of the
first-order model for iron, manganese, copper, and zinc in a water wetland in Kanata, Ontario, over a two-year period These authors found that it was acceptable for some metals (e.g., zinc) but not for others (e.g., iron and manganese) They observed that such a model could not account for releases, and might also be affected by the low concentrations that
storm-existed in the incoming water Crites et al (1997) found
exponentially decreasing profiles for zinc in water along the flow direction at the Sacramento wetlands (Figure 11.9), as indicated by Equation 11.17
One of the premier uses of mesocosm experimentation is
to control external factors, in an effort to elucidate processes
The efforts of Manyin et al (1997) assist in the
understand-ing of which model may be more realistic Side-by-side cosms were fed iron solutions of varying concentrations and at varying flow rates Data fit to Equation 11.17, across three inlet concentrations and four hydraulic loadings, produced a mean
meso-k = 53 m/yr, with R2 = 0.83 Thus, when there are not artifacts
of variable pH, temperature, flow, or ancillary chemistry, the first-order model is quite effective in describing data As a cor-ollary, the use of an area-adjusted contaminant removal rate was entirely inappropriate for these controlled conditions.Another approach to investigation of removal models relies upon the accumulation of metals in new wetland sedi-ments If for the sake of simplicity, the plug flow model
is used as a basis for interpretation, it may be shown that exponential reductions in waterborne metals along the flow path result in the appearance of exponentially distributed
0.001 0.01 0.1 1 10 100 1,000 10,000 100,000
0.001 0.01 0.1 1 10 100 1,000 10,000 100,000
Bisufide Sulfur (µg/L)
Inlet Outlet Amorphous ZnS Sphalerite ZnS
FIGURE 11.8 The reduction in zinc in an anaerobic treatment wetland in Butte, Montana, compared to MINTEQA2 forecasts for
amor-phous and mineral ZnS (Adapted from Frandsen and Gammons (2000) In Wetlands & Remediation: An International Conference Battelle
Press, Columbus, Ohio, pp 423–430.)
Trang 21top sediment accretions of those metals The buildup of
those new top sediments may be considered the result of
the wetland carbon cycle, which produces a stable annual
accretion for a fully developed wetland When combined
with Equation 11.17, the concentration in the new sediments
can be computed at each location The rate of deposition at
some fractional distance y along the wetland flow path is:
Then a mass balance on the top layer of deposited material
determines the concentration in the surficial solid layer:
J
kC J
kAy Q
y rractional distance along flow path, dimensiionless
A benefit of this analysis is that the temporal
variabil-ity of water concentrations is averaged by the sampling of
many months or years of accretion The Sacramento,
Cali-fornia, project sampled longitudinal profiles after 3.5 years
of operation (Nolte and Associates, 1998b), and designated
the new top sediments as the A layer Interpretation of the
Sacramento data was via the first-order areal model
(Dom-beck et al., 1998) Results indicated that exponential declines
explained a considerable amount of the variability in A layer
solids concentrations (Figure 11.10) Rate constants fall in the
range 22–71 m/yr Thus it appears that the first-order model
is applicable to field situations on a long-term average basis
More detailed models have been proposed, but these
gener-ally lack calibration to multiple systems A significant effort at
detailed process modeling was the development and calibration
of the Constructed Wetland Fate and Aquatic Transport ation (CWFATE) model for the Sacramento, California project (Jones & Stokes Associates, 1993; Nolte and Associates, 1998a, b) CWFATE attempts to describe water budgets, lead biomass cycles, and partitioning, but not chemical precipitation Flana-
Evalu-gan et al (1994) proposed a detailed model, and calibrated it
for iron and aluminum at the Lick Run, Pennsylvania, wetland, but this model has not gained general acceptance The PIRA-MID project developed a proprietary metals model for mine water applications (PIRAMID Consortium, 2003a)
In this chapter, system data analyses are presented for percent concentration reduction, areal removal rates, and first-order rate constants
S TORAGE IN P LANTS
Plants are a secondary location for metal storage, compared
to sediments Furthermore, most of the metal found in plants
is located in the roots and rhizomes (Table 11.15) quently, harvest of aboveground plant parts is not an effective means of removing metals from the wetland
Conse-S EDIMENT S TORAGE C ONCENTRATIONS
A Well-Mixed Surficial Zone
There are two ways to consider the buildup of stored metals
in a treatment wetland The first presumes that metal storage occurs throughout the root zone of the FWS wetland, with transfers to sediments and roots driven by processes such as sorption and transpiration flows
Additionally, wetland sediments contain a variety of organisms that ingest sediments over a wide range of depths, and redeposit their gut contents primarily at the sediment surface (Robbins, 1986) By such means, metals may reach the entire root zone layer, and continue to build up in con-centration As for other contaminants in wetlands, the major storage will be in the roots, soils, and sediments, rather than
in aboveground tissues Thus, this approach considers the root zone to be a well-mixed region, with ever increasing
y = 25.8 exp(–0.0099x)
R 2 = 0.884
1 10 100
Distance (m)
FIGURE 11.9 Profile of water-phase zinc along the flow direction in Sacramento, California, Cell 7B in May 1995 The corresponding
k = 45 m/yr (Data from Crites et al (1995) Removal of metals in constructed wetlands Proceedings of the 68th Annual WEFTEC Conference
Water Environment Federation, Alexandria, Virginia; and Crites et al (1997) Water Environment Research 69(2): 132–135.)
Trang 22424 Treatment Wetlands
solid concentrations The metal load removed contributes
to the increase, in simple form, as:
of copper was 132 mg/m2·yr The top 25 cm of the wetland contained 50 kg/m2 of dry solids (at Rb = 200,000 g/m3), and hence the rate of concentration increase was 2.65 mg/m2·yr Therefore, the increase from 27 to 35.7 mg/kg would take 3.3 years Storage lifetimes for other metals ranged from zero (TEL exceeded for baseline condition) to 120 years for lead.This calculation presumes vertical uniformity in the root zone, which is not typically observed Further, it does not include the effects of new sediment deposition, which is very common in FWS treatment wetlands Accretion, precipita-tion of metals, and downward diffusion with sorption all tend
to create layering in the upper soil sediment horizon
Managed Peat Systems
When metal concentrations are high, accumulation on ments is also high for many metals Under high loadings, the
sedi-TABLE 11.15
Fraction of Removed Metal Load Found in Plants
after Five Years of Operation
Source: Adapted from Nolte and Associates (1998b) Sacramento
Regional Wastewater Treatment Plant Demonstration Wetlands
Project: Five Year Summary Report 1994–1998 Report to Sacramento
Regional County Sanitation District, http://www.srcsd.com/cw.html ,
Nolte and Associates, Sacramento, California.
0.01 0.1 1 10 100 1,000
Distance (m)
Zn Cu As Ag Cd Hg
FIGURE 11.10 Profiles of metals in sediments along the flow direction for Sacramento, California, Cell 7 in 1997 (Data from Nolte and
Associates (1998a) Sacramento Regional Wastewater Treatment Plant Demonstration Wetlands Project 1997 Annual Report to mento Regional County Sanitation District, Nolte and Associates, Sacramento, California.) The corresponding areal k-values are:
Trang 23wetland ecosystem cannot generate enough sorption capacity
via its carbon cycle In some instances, the initial amount of
substrate may provide for a long removal lifetime For instance,
Eger and Lapakko (1989) estimated lifetimes for four wetlands
associated with nickel removal at the Dunka Mine site in
Min-nesota At hydraulic loadings of 0.12–0.60 cm/d, and nickel
concentrations of 0.9–15.4 mg/L, they estimated sorption
capacity would last 20–780 years In other cases, there may
be a need to replenish the sorbent on a more frequent basis In
the wetland environment, that means digging out the substrate
and finding appropriate means of disposal Operational and
maintenance costs so incurred must then be considered in the
evaluation of a project The alternative of using the peat as a
sorbent in a controlled, mechanical apparatus should then be
considered (Coupal and Lalancette, 1976; Sharma and Forster,
1993; Brown et al., 2001; Fine et al., 2005).
The “Layer Cake” Assumption
The second way to interpret metal storage in FWS wetlands is
to presume that all the current storage is contained in a newly
formed top sediment layer, which does not mix with
previ-ous layers (Kadlec, 1998) This is a limiting concept, because
there is very likely to be some sediment metal mixing as a
result of bioturbation and vertical chromatographic flows
Vertical stratification of FWS treatment wetland sediments/
soils usually includes a top-most floc layer, which has been
described as “a slurry of dark, decomposing, loosely structured
detrital material that pours out when the sampler is tipped” and
termed the A layer (Nolte and Associates, 1997) This layer has
been observed in a range of treatment wetland types, ranging
from those receiving secondary effluent in Sacramento,
Cali-fornia, to those receiving agricultural runoff in South Florida
(SFWMD, 2006) The thicknesses are about 5–30 cm; for
instance, 11.3 o 2.7 cm along the flow direction at Sacramento
Cell 7 in 1996 Below this floc, there may be a second layer
dominated by litter and sediment, termed the B layer by Nolte
and Associates (1997) This B layer averaged 4.6 o 1.0 cm for
Sacramento Cell 7 in 1996 Below this, there existed a C layer
of gleyed clay soil at Sacramento, in turn atop the base clays
of the wetland basins The metals content of these various ers were found to be markedly different, with 2–13-fold higher
lay-concentrations in the A layer than the C layer (Figure 11.11) It
is probable that the layering pattern in concentrations is driven
by processes of precipitation and sorption
Metal storage in the top layer creates sustained sediment concentrations that reflect the dilution of new metal deposits
by the accretion of new wetland solids Such accretions result from microbial, algal, and macrophyte detritus production, and lead to replacement of floc layers, which are depleted by consolidation In a sense, this concept amounts to plug flow
of metals and biomass downward into the top sediments, or
“conveyor-belt” deposition Under this assumption, a mass balance on the top layer of deposited material determines the concentration in the surficial solid layer:
J
S metal
sed
where
C J
S meta
top layer solid concentration, mg/g
J ssediment accumulation rate, g/m ·yr2
For example, consider Jsed = 200 dry g/m2·yr of new ments, originating from 1,000 dry g/m2·yr of biomass
sedi-production Suppose the metal removal rate is Jmetal = 10 mg/
m2·yr When this metal stream is diluted by the new ment stream, a new, top sediment concentration of 50 µg/g (0.05 mg/g) is forecast This may then be compared to the appropriate sediment quality criterion for the metal in ques-tion This example may be continued to estimate the corre-sponding water concentration:
k
For the example under consideration, if the value of k =
50 m/yr, then C = 0.2 mg/m3 (µg/L) From the magnitudes of
0.01 0.1 1 10 100 1,000
Layer A Layer B Layer C
FIGURE 11.11 The vertical layering effect on average sediment metal concentrations in the first 100 m of Sacramento, California, Cell 7
(Data from Nolte and Associates (1998a) Sacramento Regional Wastewater Treatment Plant Demonstration Wetlands Project 1997 Annual
Report to Sacramento Regional County Sanitation District, Nolte and Associates, Sacramento, California.)
Trang 24426 Treatment Wetlands
the numbers in this hypothetical example, it is easily seen that
if the wetland is effective, and there is elevated metal in the
incoming water, it will be difficult to meet stringent sediment
quality standards (Kadlec, 1998)
11.6 THE OXIDE FORMERS
I RON
Iron is a metal that may occur at trace to high concentrations in
wetland surface waters and sediments It is required by plants
and animals at significant concentrations In plants, iron is an
essential element in chlorophyll synthesis, cytochromes, and
in the enzyme nitrogenase In animals, iron is important in
oxidative metabolism and is a key component in hemoglobin
Iron at low to moderate concentrations is not generally
regarded as a threat to human health or aquatic life The U.S
EPA has recommended a continuous concentration criterion of
1,000 µg/L for protection of freshwater aquatic environments,
and a drinking water human health criterion of 300 µg/L
(U.S EPA, 2002b) The province of Ontario, Canada, has a
lower standard for protection of aquatic life, also 300 µg/L
Perhaps the greater concern is for the blanketing effect of
thick deposits of iron precipitates in wetlands designed to
treat high iron concentrations (Kelly-Hooper, 1999)
High concentrations of soluble iron in surface water and
wetland systems may result from natural or artificial iron
sources, typically as seeps of ferrous iron and iron sulfides
(pyrites) from anaerobic groundwaters Iron bacteria that
pro-duce ocher, such as Leptothrix ochracea and Spirophyllum
ferrugineum, derive their energy needs from the oxidation of
reduced iron These bacteria typically occur in wetland areas
where anoxic waters meet aerated surface conditions, such
as upwelling springs or other venting groundwaters At such
locations, reddish brown flocculent deposits form
Iron in the wetland waters may be dissolved or
partic-ulate Most reported wetland studies do not specify which
forms were determined This may be a critical unresolved
issue, because there may be very large amounts of suspended
iron in wetland waters Gammons et al (2000b) report that
the iron concentrations between filtered and unfiltered
sam-ples can differ by a factor of up to 100 Their data may be
approximated as unfiltered iron equal to the square root of
filtered iron, over the range 10–5,000 µg/L
Wetland Storage and Processing of Iron
In an oxygenated environment, ferric iron is present as
insol-uble oxyhydroxides, denoted as FeOOH If there is not
suf-ficient alkalinity in the water, the reaction produces acidity:
However, if there is sufficient alkalinity, removal of iron to
precipitates is not accompanied by a decrease in pH:
31
12
The water is deemed acidic for iron removal if the ratio
of iron to CaCO3 alkalinity is greater than 1.1 (Younger et al.,
2002)
Oxidation and reduction of iron occurs relatively ily depending on redox potential and pH (Faulkner and Richardson, 1989) Fe3+, or ferric iron, is the dominant form under oxidized conditions (Eh > 0 at pH q 6.5) Fe2+, or fer-rous iron, is the dominant form under reduced conditions
eas-in wetlands and other aquatic environments Fe3+ forms stable complexes with a variety of ligands It joins with the hydroxide ion in surface waters to form reddish-brown ferric hydroxide (Fe(OH)3), which is also known as ocher Ocher
is insoluble and either settles to the bottom sediments or remains in suspension, adsorbed to living and dead organic matter (see Figure 7.10) Other important compounds formed
by ferric iron include ferric phosphate (FePO4), iron-humate complexes, and ferric hydroxide-phosphate complexes.Ferric iron is reduced to the ferrous form under anaerobic conditions The ferrous iron is more soluble, resulting in the release of dissolved iron and associated anions such as phos-phate from anaerobic sediments in wetlands The formation
of this soluble ferrous iron may be controlled somewhat by sulfide, which forms the relatively insoluble ferrous sulfide (FeS) Sulfide formation is written as:
The required HS– is microbially generated, and occurs preferentially in organic environments by the reduction of sulfate (see Equations 11.1, 11.2, and 11.3)
The role of sulfate-reducing bacteria (SRB) in the cycling
of iron and sulfur was studied in a young constructed wetland
located in Kanata, Ontario, Canada (Fortin et al., 2000)
Sedi-ments and water samples were collected over the course of one year within each of three FWS cells SRB populations were largest during the cold winter months, when the temperature
of the water was 1°C The presence of high-SRB populations also corresponded to highly anoxic conditions within the sedi-ments and to a decrease of sulfate concentrations, suggesting that cold temperature did not affect the activity of SRB The results indicated that iron and sulfur cycling in the constructed wetland was active throughout the year, especially in the cold winter months This suggests that iron removal in wetlands can be effective in temperate climates, even though the tem-perature of the water decreases drastically during the winter
Soils and Sediments
Wetland soils can contain large amounts of iron, especially when exposed to metalliferous waters (Table 11.16) On a dry basis, ferric oxide contains 70% iron by weight (700,000 mg/kg), and this represents an upper limit to sedimentary iron concentrations in oxic wetland waters Iron sulfides contain 53% (FeS2) and 66% (FeS) iron Such mineral precipitates are diluted by newly formed organic materials in the wetland
Trang 25environment, and lesser concentrations are observed For
ins-tance, Doyle and Otte (1997) measured 6,000–40,000 mg/kg,
and higher values in the rhizosphere and near worm burrow
walls
Freeze-coring and analysis of the wetland substrates
indi-cated that total sulfur was present in three forms, in the following
proportions (Younger, 2000): FeS: 35%; FeS2: 31%; S°: 34%
On the basis of these observations, it was postulated that
pH rise was due to the consumption of protons via reactions
involving reduction of ferric hydroxide and precipitation of
elemental sulfur The removal of iron from solution and
for-mation of significant quantities of S° is consistent with the
following coupled reactions:
Goulet and Pick (2001) found that the presence of cattails had
little effect on the partitioning of iron in shallow wetland
sed-iments in FWS wetlands Studies at four Ontario treatment
wetlands showed total iron in the sediments of 2,000–12,000
mg/kg, with sediment organic content of 8–20% About half
of the sediment iron was in reactive forms, oxides,
monosul-fides, or sorbed on organic matter The balance was
domi-nated by forms associated with either the pyrite (one wetland)
or the silicate fraction of the sediment (three wetlands)
Wetland Plants
Metals reach plants via their fine root structure, and most
are intercepted there Some small amounts may find their
way to stems, leaves, and rhizomes Upon root death, some
fraction of the metal content may be permanently buried, but there are no data on metal release during root decomposition However, wetland plants bring oxygen to their root zone to maintain respiration, and some fraction is lost by radial dif-fusion away from the roots This creates small aerobic zones near the roots, in which iron precipitates may form These
are termed iron plaque.
Nonetheless, some iron is taken up into aboveground sues Iron occurs in wetland plants at concentrations rang-ing from about 200–2,000 mg/kg dry mass (Vymazal, 1995) Plant roots contain a much higher concentration of iron than stems or leaves (Table 11.17) Uptake by plants and algae may
tis-be for purposes of growth enhancement, or at higher metal concentrations for protective purposes Biomagnification of iron does not occur
A common concept of wetland treatment is the perceived risk of seasonal release of contaminants during winter, when wetland macrophytes die back This theoretical risk was investigated experimentally in mesocosm experiments on plant litter collected from long-established mine water treat-ment wetlands in the United Kingdom (Batty and Younger, 2002) Metals were not released from the plant litter; and iron concentrations in the litter increased after 6 months of decomposition, which was attributed to adsorption Field studies undertaken within the PIRAMID project (PIRAMID Consortium, 2003a) found that wetlands were net sinks for iron in all seasons
Performance of Wetlands for Iron Removal
Wetlands interact strongly with iron in a number of ways, and thus are capable of significant metal removal Three major mechanisms are operative:
TABLE 11.16
Iron Content of Top Sediments in a Variety of Wetlands
Iron
Panel, Ontario Cattail marsh Urban stormwater 12,000 Goulet and Pick (2001)
Monahan, Ontario Cattail marsh Urban stormwater 2,500 Goulet and Pick (2001)
Falconbridge, Ontario Cattail marsh Acid mine drainage 1,500 Goulet and Pick (2001)
Riverwalk, Ontario Cattail marsh Tailings leachate 1,500 Goulet and Pick (2001)
West Page Swamp, Idaho Cattail, Arrowhead Tailings leachate 115,500 DeVolder et al (2003)
Widows Creek, Alabama Cattail, Juncus Tailings leachate 60,000–85,000 Ye et al (2001a,b)
Show Low, Arizona Pintail marsh Municipal 30,575 NADB database (1998)
Tres Rios, Arizona Four wetlands Municipal 18,857 Wass, Gerke, and Associates (2002)
Sacramento, California Seven wetlands Municipal 17,096 Nolte and Associates (1998)
Champion Paper, Florida Pilot Pulpand paper 9,400 NADB database (1998)
Monroe Co., New York Pilot Leachate 2,560–2,720 Eckhardt et al (1997)
Poland 11 lakes Brown coal pits 115–21,500 Samecka-Cymerman and Kempers (2001)
Trang 263 Uptake by plants, including algae (however, after
the plant senescence or algal die back most iron is
leached out)
Information on the effects of wetlands on iron
concentra-tions has been reported at a low level of detail, with emphasis
on removal percentages Three principal categories of influent
waters are mine drainage, landfill leachates, and municipal
wastewater Mine drainage control dominates the applications,
with well over a hundred systems in place and reporting data by
1990 (Weider, 1989) Many landfill leachates contain enough
iron to induce monitoring of wetland systems built for
leach-ate improvement Iron is not typically monitored in municipal
wastewater wetlands, and there are but few data sets that exist
Example performances are shown in Table 11.18 Inflow
and outflow concentrations vary over 1,000-fold Removal
percentages are high for mine waters and leachates, but lower
or negative for waters with low iron content SSF systems,
due to prevailing anoxic/anaerobic character of the filtration
bed, usually do not perform well in terms of iron removal
The filtration bed becomes more anaerobic over the period
of operation and majority of iron is reduced to more soluble
ferrous compounds which are washed out of the system
If hydrogen sulfide is present as a consequence of sulfate reduction (Equations 11.1 and 11.2), iron may form insoluble ferrous sulfides (Equation 11.27) and is deposited in the bed
Coal Mine Drainage Wetlands
Information on iron removal in wetlands is available ily from acid mine drainage (AMD) wetland treatment sys-
primar-tems in the United States (Girts et al., 1987; Kleinmann and
Hedin, 1989; Hedin, 1989) However, treatment wetlands also became widely used in the United Kingdom in the 1990s Younger (2000) lists 24 wetland systems, which fall into two principal categories:
Aerobic FWS wetlands, usually vegetated by Phragmites australis These are typically used for
iron reduction in net-alkaline waters
FWS with an anoxic compost substrate, typically vegetated by Phragmites australis Because of the
organic substrate, these are called anaerobic FWS wetlands These are typically used for iron reduc-tion in more acidic waters
Of the 137 AMD wetland treatment sites reviewed by Wieder (1989), 66% had influent iron concentrations less than
50 mg/L An average total iron concentration of 60.6 mg/L was reduced to an average outflow concentration of 15.4 mg/L,
•
•
TABLE 11.17
Iron Content of Above- and Belowground Plant Parts in a Variety of Wetlands
Above (µg/g)
Below
TVA Mussel Shoals, Alabama FWS CW Typha spp. 45–142 1,011–7,437 NADB database (1998)
Widows Creek, Alabama FWS CW Typha latifolia 1,217 68,469 Ye et al (2001a,b)
Coeur d’Alene, Idaho FWS Nat Typha latifolia 200 — DeVolder et al (2003)
11 lakes, Poland FWS Nat Typha angustifolia 350 — Samecka-Cymerman and Kempers (2001) TVA Mussel Shoals, Alabama FWS CW Phragmites australis 112–161 2,533–4,547 NADB database (1998)
Nucice, Czech Republic SSF CW Phragmites australis 139 — Vymazal and Krása (2005)
New York FWS CW Phragmites australis 618–799 7,060–9,280 Eckhardt et al (1997)
Br˘ehov, Czech Republic SSF CW Phragmites australis 74 3,677 Vymazal et al (2006)
11 lakes, Poland FWS Nat Phragmites australis 1,053 — Samecka-Cymerman and Kempers (2001) TVA Mussel Shoals, Alabama FWS CW Phalaris arundinacea 89–309 2,445–8,352 NADB database (1998)
Nucice, Czech Republic SSF CW Phalaris arundinacea 323 — Vymazal and Krása (2005)
Br˘ehov, Czech Republic SSF CW Phalaris arundinacea 70 3,383 Vymazal et al (2006)
11 lakes, Poland FWS Nat Phalaris arundinacea 1,202 — Samecka-Cymerman and Kempers (2001) TVA Mussel Shoals, Alabama FWS CW Scirpus acutus 47–107 1,820–2,754 NADB database (1998)
TVA Mussel Shoals, Alabama FWS CW Scirpus cyperinus 83–723 1,185–2,228 NADB database (1998)
11 lakes, Poland FWS Nat Scirpus lacustris 430 — Samecka-Cymerman and Kempers (2001) Widows Creek, Alabama FWS CW Juncus effusus 320 41,318 Ye et al (2001a,b)
Coeur d’Alene, Idaho FWS Nat Sagittaria latifolia 220 — DeVolder et al (2003)
Note: FWS = free water surface; SSF = subsurface flow; CW = constructed wetland; Nat = natural wetland
Trang 27for an average iron removal efficiency of 58.2% and a median
value of 80.9% (Wieder, 1989) This median is clearly also
close to that experienced at the U.K sites (Table 11.18) This
treatment efficiency was found to weakly correlate directly
with wetland area and inversely with wetland depth An
aver-age iron removal rate of 3,650 kg/hayr at pH 6 in AMD
treat-ment wetlands was given by Kleinmann and Hedin (1989)
Because the iron removal rate is correlated with iron
load-ing rate (Hedin and Nairn, 1990), lower removal rates are
expected at low influent concentrations
Landfill Leachate Wetlands
Scrap iron items discarded to landfill create an underground
source of iron, which then appears as a constituent of
leach-ate Raw leachate concentrations may be as high as 500 mg/
L, mostly in soluble form because of the anaerobic condition
of the water in the pile (McBean and Rovers, 1999) At such
high concentrations, iron precipitates pose a serious
clog-ging threat even for FWS wetlands Consequently, aeration
and precipitation are often included as pretreatment steps
(Hoover et al., 1998; Loer et al., 1999)
Oxidation/precipita-tion basins are open water impoundments designed to
pro-vide aeration for precipitation of aqueous iron, detention
time to settle precipitates, and storage volume for lating precipitate sludge These basins are a key component
accumu-in passive systems where iron is present A detention time of
at least 24 hours is recommended to produce a clear water
discharge (Hoover et al., 1998) The leachates in Table 11.18
all had lower iron than that in raw leachates due to aeration basin pretreatment or dilution
FWS wetlands produce considerable further reduction
in iron, with a median removal of 85% for the six systems
in Table 11.18 Subsurface systems may also be used For
instance, Surface et al (1993) measured an iron removal
effi-ciency of 78.6% in a HSSF wetland planted with common
reed Bulc et al (1997) reported an iron removal of 80% in
a landfill leachate HSSF system in Slovenia with outflowing concentration of 10 mg/L
Other Water Sources
A variety of other wastewaters have been subjected to wetland treatment, and in some few cases the iron content of inflows and outflows has been measured This is usually ancillary monitor-ing, which does not target regulatory requirements Byekwaso
et al (2002) found the iron reduction of 27% in a FWS-HSSF
system in Uganda treating cobalt extracting wastes The iron
TABLE 11.18
Removal of Iron in Constructed Wetlands
Inlet (mg/L)
Outlet (mg/L)
Reduction (%)
Removal (g/m 2 ·yr) Reference FWS
Eleven Systems United Kingdom Coal mine water 19.6 2.53 87 — Younger (2000)
Ten Systems Tennessee Valley Coal acid mine 58.3 9.36 82 1,028 Brodie (1990)
Albright Pennsylvania Coal mine water 2.45 0.33 87 56 Hoover et al (1998)
Springdale Pennsylvania Coal mine water 12.46 0.27 98 436 Hoover et al (1998)
Musselwhite Ontario Metal mine water 0.155 0.038 75 22 Bishay and Kadlec (2005)
Kanata Monahan Ontario Metal mine water 0.36 0.27 25 11 Goulet and Pick (2001)
Elliot Lake Panel Ontario Metal mine water 15 0.3 98 141 Goulet and Pick (2001)
New Hanover County North Carolina Leachate 1.746 0.134 92 1.3 Unpublished data
Estevan Saskatchewan Municipal lagoon 0.296 0.197 33 1 Unpublished data
Twelve Systems Arcata, California Municipal lagoon 0.60 0.55 8.3 2 NADB database (1998)
Six Systems Champion, Florida Pulp and paper 0.330 0.530 NADB database (1998)
Orange Eastern Orlando, Florida Municipal 3° 0.017 0.067 NADB database (1998)
Tres Rios Phoenix, Arizona Municipal 3° 0.200 0.233 Wass, Gerke, and Associates (2002)
HSSF
Median HSSF
Trang 28430 Treatment Wetlands
content of pretreated municipal wastewater is likely to be less
than 1 mg/L in many regions, although higher in regions with
high occurrence of iron minerals (Table 11.18) For example,
Vymazal (2003) reported reduction of Fe from 1.1 to 0.72 mg/L
in a HSSF system treating municipal sewage near Prague in
the Czech Republic However, other studies from the Czech
Republic (Table 11.18) showed rather negative removal effects
for HSSF systems due to conditions discussed above When
iron concentrations are very low, the use percent removal is no
longer an appropriate measure, because very small excursions
in concentration can greatly affect the percentage
Nonethe-less, removals may or may not occur for very low iron content
waters (see Table 11.18)
Examples and Models for Iron Removal
in Treatment Wetlands
It is likely that wetland removal performance in FWS
sys-tems is area-specific (Younger et al., 2002), rather than
vol-ume-specific Three simple predictive approaches have been
suggested:
Constant percent removal Specification of a
sup-posedly constant percentage removal
Zero-order removal Specification of a supposedly
constant areal removal rate, in g Fe/m2·d This
cor-responds to zero-order removal kinetics, for which
removal is independent of the iron concentration
First-order removal The reduction rate is
pro-portional to the iron concentration (Tarutis et al.,
1999) Some of the contributing processes are
first-order, such as oxidation of ferrous iron and
bacte-rial sulfate reduction (Younger et al., 2002), as is
the process of particulate settling of precipitates
However, global removal does not necessarily
fol-low such a model
Data from 35 FWS natural wetlands receiving inputs of
fer-ruginous acid mine drainage in western Pennsylvania served
as a basis for evaluating the merits of these three approaches
•
•
•
Stark and Williams (1995) found that percentage removal was
a better index of treatment than areal removal Nevertheless, a fixed areal removal rate of 10 g Fe/m2·d remains the accepted design guideline for high levels of removal, while 20 g Fe/m2·d
is allowable to cause considerable improvement (Hedin et al.,
1994; PIRAMID Consortium, 2003a)
Tarutis et al (1999) further analyzed the 35-wetland
data set, and concluded that percentage removal should not
be used, and that areal removal did not separate the effects
of inlet concentration and flow rate They recommended the first-order model (Equation 11.17), and found a median rate constant of 0.18 m/d (66 m/yr) (N = 35) for calibrations of a plug flow version of the model
Manyin et al (1997) performed a factorial experiment
varying flow rate and inlet concentrations to wetland cosms They found that outlet iron concentrations increased with increasing inlet iron loadings Analysis of their data pro-duces a rate constant of 42 m/yr according to Equation 11.17.More complex models have been proposed, but these have not yet reached a point of usefulness in wetland design
meso-For instance, the proposed model of Flanagan et al (1994)
presupposes that removal is to sulfides, and contains no mentation step for ferric oxyhydroxides Modeling software has been developed allowing simulation wetland systems (NOAH2D) (PIRAMID Consortium, 2003b) NOAH2D sim-ulates overland flow and solute transport through reed beds, allowing for frictional resistance to flow offered by wetland vegetation, and also allows for exchange with (and hyporheic flow within) permeable wetland bed sediments This code
sedi-is a research tool, rather than software available for design The complexity of the NOAH2D code requires very long run times, and full calibration is acknowledged as unlikely by the
authors (Younger et al., 2002).
The Manyin et al (1997) findings suggest the use of a
graphical representation of wetland effluent iron versus inlet iron loading These variables are completely independent, and avoid the artifact of spurious correlations caused by the inclu-sion of a common factor in both ordinate and abscissa Infor-mation from 46 constructed wetlands was used to form such a
0.01 0.1 1 10 100
Iron Load In (g/m 2 yr)
Other Coal Mine Water Leachate
Manyin et al Mesocosms
FIGURE 11.12 Outlet iron concentrations from FWS wetlands at various loading rates.
Trang 29display (Figure 11.12), together with the Manyin et al (1997)
mesocosm data There are two zones apparent on this graph:
above about 100 g/m2·yr loading, there is an increase in outlet
iron with increased iron loading; below about 100 g/m2·yr
loading, there is a much more gradual increase in outlet iron
with increased iron loading The 100 g/m2·yr loading also
represents the maximum that may be imposed without
wet-land effluent concentrations exceeding 1 mg/L The k-values
previously cited were not determined or verified for the low
loading region
In the low loading region, behavior probably reflects
localized recycling of iron to and from precipitates and
adsorbed forms, in response to localized variations in pH
and mediated by diffusion to and from the water column
Background levels may also result from suspended
particu-late forms of iron Uptake into aboveground macrophyte
plant parts is low, but larger amounts of iron are found in
roots, so that overall plant cycling can be of importance
Batty and Younger (2002) found that where dissolved iron
concentrations in wetland waters were at or below 1 mg/L,
direct uptake of iron by plants could account for 100% of
iron removal This finding explained why aerobic reed-beds
removed dissolved iron at far greater rates than would be
anticipated on the basis of the first-order kinetics of Fe2+
oxi-dation Batty and Younger (2002) also found 1 mg/L iron was
also an optimum for healthy growth of Phragmites australis:
at greater concentrations, the plants were not as productive,
while at lower concentrations were healthy
Variability of Iron Removal in Treatment Wetlands
Intersystem variability in the Stark and Williams (1995)
data sets was relatively high, with removal of 64% o 28%
(mean o SD) It was less in the Manyin et al (1997)
cosms, with removal of 89% o 13% (mean o SD) The
meso-cosms were operated in the laboratory, and had no variability
in depth, aspect ratio, weather conditions, or substrate; and
were all operated at circumneutral pH
Intrasystem variability has not been reported for
continu-ous flow wetlands, but it is high for event-driven wetlands
For example, the coefficient of variation of outlet iron from
the Hidden River wetland in Florida was 4.7 (ASCE, 2003)
Summary
Iron is effectively removed by treatment wetlands over the
high end of the concentration range, which is typical of acid
mine drainage and landfill leachates Rates are rapid, and
significant loadings may be removed At low concentrations,
and loadings below 100 g/m2·yr, iron cycling creates low
con-centrations in the water column Removal is to precipitates,
either oxyhydroxides or sulfides Accumulation of these
materials is a factor in the ecological status of the wetland
A LUMINUM
Aluminum occurs naturally in surface waters, to a small extent
in the hydrated ionic forms, and to a greater extent complexed
with silicates in a colloidal form Aluminum solubility varies with pH It is least soluble at a pH of 7 and increases in solu-bility as Al3+, Al(OH)2+, and Al(OH)2 ions at 4 < pH < 5; and
as aluminate ion Al(OH)4 at pH > 9 (Gensemer and Playle, 1999) Aluminum precipitates as amorphous Al(OH)3, which
may slowly form the mineral Gibbsite (Berkowitz et al.,
2005) Precipitation is rare in natural waters, but is of interest
in treatment processes that rely upon addition of aluminum chlorides or sulfates for purposes of phosphorus removal
Wetland Processing and Storage of Aluminum
Aquatic systems typically contain low concentrations of total aluminum In the Adirondacks region of the eastern United States, 203 lakes had a mean pH = 6.3, and a mean total Al =
138 µg/L In Florida, 168 lakes had mean pH = 6.3 and a mean total Al = 89 µg/L Lakes are typically net sinks for aluminum, with 10–50% retention for low pH, and 70% for circumneutral conditions (Gensemer and Playle, 1999) Organic complex-ation occurs in natural waters, as binding to humic substances Trivalent cations such as Al3+ are more susceptible to binding
to organic ligands than divalent cations Peat based wetlands often provide the conditions of low pH that foster Al3+, and hence dissolved organic matter, or dissolved organic carbon, is
an important factor in wetland aluminum water chemistry.Aluminum is toxic to many species of algae, with effects being observed over a range of a few hundred to a few thousand µg/L total aluminum However, aquatic invertebrates are much less affected, and do not biomagnify aluminum Wetland mac-rophytes are tolerant of high aluminum concentrations, in the thousands of µg/L total aluminum Salmonid fish are suscep-tible to a variety of effects for concentrations of a few hundred
to a few thousand µg/L U.S EPA (1988a) ambient water ity standards are 87 µg/L (chronic) and 750 µg/L (acute), but research is currently in progress to improve these numbers
qual-Aluminum uptake by emergent and floating plants (Typha and Lemna) was found mainly into the roots and rhizomes (Goulet et al., 2005) In contrast, there was no clear pattern for submerged plants (Utricularia and Potamogeton) Roots also
had the highest aluminum concentrations at the Tres Rios, Arizona, treatment wetlands (Table 11.19; Wass, Gerke, and Associates, 2002) Sediments generated in treatment wetlands are often high in aluminum, with values in treatment wetlands ranging from 1.4% (Tres Rios, Arizona) to 4% (Sacramento, California) (Nolte and Associates, 1998b)
The process of phosphorus adsorption onto aluminum hydroxides has seen extensive application to water treatment and lake eutrophication management as a means of control-ling excess dissolved phosphorus Alum or polyaluminum chloride additions are designed to form a floc of insoluble Al(OH)3, which in turn adsorbs phosphorus In wetlands, without coagulation, this floc settles slowly or not at all, leaving particulate aluminum and phosphorus in suspension (Bachand and Richardson, 1999) However, alum addition is
a pretreatment step for waters sent to wetlands for further polishing Wetlands are also the recipients of water treatment
backwash and sludge (Kaggwa et al., 2001) Consequently,
Trang 30432 Treatment Wetlands
aluminum is sometimes a contaminant in treatment wetland
influents, either by intentional or accidental discharges
Aluminum is a strong determinant of the phosphorus
adsorption capacity in wetland soils (Reddy and D’Angelo,
1994) The phosphorus adsorption process in treatment
wet-lands is a temporary mechanism, which is exhausted when
all antecedent soil sorption sites are used However, the
amount of phosphorus that may be bound to wetland soils
forms an important part of the wetland start-up capacity for
phosphorus removal A phosphorus removal project has been
implemented using aluminum sludge from a water treatment
plant as a soil amendment (SAIC, 2005)
There are two main groups of projects that have
mea-sured aluminum removal in wetlands:
FWS wetlands, which typically receive low
con-centrations and loads of aluminum
SSF wetlands, which, for aluminum, typically
treat acid mine waters with quite high
concentra-tions and loads
Aluminum Removal Processes
Mine waters with pH less than 4 commonly contain high
concentrations of aluminum (>10 mg/L) (Younger et al.,
2002) Aluminum is present as trivalent Al, and the currently
accepted removal reaction is:
3
The precipitate is amorphous, white, and of low density It
may later crystallize to gibbsite These solids are common
components of many natural soils, and pose no problem as
new wetland sediments and soils (Younger et al., 2002) In
the presence of dissolved sulfate, hydroxysulfate precipitates
may form as well
Performance of Wetlands for Aluminum Removal
Examples of wetland reductions in concentration and mass
removals are shown in Table 11.20 Performance is variable
•
•
across systems, with a median concentration reduction of 50% Wieder (1989) examined 20 acid mine wetlands for reductions, and found a median of 47.7%, and a 75th percentile of 78.9% Wieder (1989) also found one quarter of the acid mine wet-lands had zero reduction Vymazal and Krása (2003) reported decrease of aluminum concentration from 451 μg/L to less than 40 μg/L in a 62-m long HSSF constructed wetland in the Czech Republic The major decrease (from 451 μg/L to 65 μg/L) occurred within the first 15 m of the bed Other results from HSSF wetlands treating municipal wastewater (Table 11.20) exhibited good removal of aluminum (53–90%)
Removal is to accretion in sediments, which form a source of potential return fluxes of aluminum, most likely
as particulates In a mesocosm study, Wieder et al (1990)
found that although aluminum was initially removed in a wetland, this process decreased with time, and the wetland
began to export aluminum to downstream waters Wieder et
al (1990) found aluminum concentrations of 10 mg/L were
found to be toxic to cattails, leading to their mortality and
release of sorbed aluminum Wieder et al (1988) found the
total aluminum content of the peat increased from 2,375 to 13,634 mg/kg dry mass, with the majority bound as organic and oxide compounds
Flanagan et al (1994) proposed a model for wetland
treatment of iron and aluminum in acid mine drainage, but its utility has apparently not been tested for aluminum (Mitsch
and Wise, 1998) Regarding aluminum, Younger et al (2002)
conclude that much remains to be investigated in detail
Example Treatment Wetlands for Aluminum Removal
There are but few data sets on the removal of aluminum from types of incoming water other than acid mine drainage (Table 11.20) Bachand and Richardson (1999) conducted field mesocosm studies on aluminum dosing to foster phosphorus removal in treatment wetlands in south Florida The “pin flocs” generated did not settle effectively Another FWS wetland study tested the concept of phosphorus removal via aluminum dosing
of agricultural runoff, but with coagulation before sending the
TABLE 11.19
Aluminum Concentrations in the Tissues of Wetland Plants in a Municipal Wastewater Treatment Wetland
(mg/kg)
Roots (mg/kg)
Reference
Three square bulrush Scirpus olneyi 12 214 Wass, Gerke, and Associates (2002)
Pennywort Hydrocotyle spp. 28 254 Wass, Gerke, and Associates (2002)
Soft stem bulrush Scirpus validus 11 168 Wass, Gerke, and Associates (2002)
Common reed Phragmites australis 39 2,177 Vymazal et al (2006)
Common reed Phragmites australis 103 — Samecka-Cymerman and Kempers (2001)
Reed canarygrass Phalaris arundinacea 1,578 — Samecka-Cymerman and Kempers (2001)
Reed canarygrass Phalaris arundinacea 43 2,584 Vymazal et al (2006)
Narrow-leaved cattail Typha angustifolia 54 — Samecka-Cymerman and Kempers (2001)
Giant bulrush Scirpus lacustris 82 — Samecka-Cymerman and Kempers (2001)
Trang 31Examples of Aluminum Removals in Treatment Wetlands
In (µg/L)
Out (µg/L)
Reduction (%)
In (kg/ha·yr)
Out (kg/ha·yr)
Removal (kg/ha·yr)
Removal (%) Free-Water Surface
South Florida STC Dosed Al-Dosed agricultural runoff 18,834 19 100 6,187 6 6,181 100 South Florida NTC Dosed Al-Dosed agricultural runoff 31,536 51 100 10,360 17 10,343 100 Friendship Hill, Pennsylvania Acid mine water 50,000 35,000 30 — — — —
Subsurface Flow
Keyser’s Ridge, Maryland Acid mine water 49,600 9,020 82 — — — —
© 2009 by Taylor & Francis Group, LLC
Trang 32434 Treatment Wetlands
water to FWS wetlands (CH2M Hill, 2001a) Aluminum was
passed to the wetlands in varying amounts, and accumulated
in the sediments Good removal from the water was observed
for the year-plus duration of the study, but a moving sediment
front appeared to have developed Undosed control wetlands
had very low levels of aluminum both entering and leaving
Water treatment alum sludge entered a wetland in Uganda,
and was effectively removed to the sediments (Kaggwa et al.,
2001) Sediment accretion was selectively higher in the inlet
region of the wetland
The aluminum industry employs FWS treatment
wet-lands in Kentucky to treat a mixed effluent from a metal
pro-cessing plant (Rowe and Abdel-Magid, 1995) Over 90% of
the aluminum is removed, from an entering level of 1.5 mg/L
Metal mine water was stripped of small quantities of
alu-minum in a FWS wetland in Ontario (Bishay and Kadlec,
2005), with reduction from 34 to 4 µg/L About two thirds
of the aluminum was removed from urban stormwater by a
FWS in Florida (Harper et al., 1986) Over 90% of the
alu-minum in a municipal wastewater was removed in a HSSF
wetland in the Czech Republic (Vymazal and Krása, 2005)
Another coal industry wastewater is the leachate
gener-ated from combustion products waste piles These waters
have much less aluminum than acid mine drainage (0.6–0.9
mg/L), and only slightly acidic pH Studies supported by the
Electric Power Research Institute (EPRI) in Pennsylvania
found that 70–90% of aluminum was removed in FWS
wet-lands (Hoover et al., 1998; Rightnour and Hoover, 1998).
Based on this limited data, it appears that aluminum
typi-cally is removed from surface water passing through wetlands
M ANGANESE
Manganese is an essential element that is chemically similar
to iron in its behavior in surface waters Manganese is vital
to plant photosynthesis and is used as an enzyme cofactor for
respiration and nitrogen metabolism by plants and animals
Although manganese is toxic to some organisms at elevated
concentrations, this situation occurs infrequently, typically
with mining wastes Manganese concentrations greater
than 2 mg/L were found to be toxic to algae in laboratory
experiments (Goldman and Horne, 1983) Manganese is not
observed to bioconcentrate in the wetland food chain
Manganese may exist in oxidation states ranging from
−3 to +7, but the manganous (+2) and manganic (+4) forms
are the most important in aqueous systems (Wetzel, 1983)
At low redox potentials and low pH the predominant form
is Mn(II) (Figure 11.13) The mineral forms are pyrolusite
(MnO2), hausmanite (Mn3O4), rhodochrosite (MnCO3), and
manganite (MnOOH) Manganous manganese can form
soluble complexes with bicarbonate, sulfate, and organic
compounds Under reducing conditions, manganese forms
insoluble complexes with carbonate, sulfide, and hydroxide
Wetland Processing and Storage of Manganese
In an oxygenated environment, manganese is primarily
removed from solution by oxidation and hydrolysis (Sikora
et al., 2000; Younger et al., 2002):
21
Abiotic oxidation of Mn(II) is very slow, and the process
is generally considered to be biologically mediated, by ria, fungi, and algae Carbonate may be an intermediate, but likely as substituted dolomite (Ca,Mg,Mn)CO3 rather than
bacte-the mineral rhodocrosite (Younger et al., 2002) Because
manganese is soluble at acidic pH, there is not a ity for manganese precipitation in acidic waters As a result, most of the removed manganese is extractable by weak acid
possibil-(e.g., 85%; Wildeman et al., 1993b).
The oxidation of manganese may be inhibited in the presence of large amounts of iron, because iron exerts a pref-erential claim on available oxygen (Hedin and Nairn, 1993):
be above neutral for this process (Figure 11.13) (Wildeman
et al., 1993b).
–200 0 200 400 600 800
MnCO3
Mn3O4MnOOH
FIGURE 11.13 Approximate distribution of manganese species
Second Edition, Academic Press, Philadelphia; and Sikora et al (2000) Water Environment Research 72(5): 536–544 Reprinted
with permission.)
Trang 33A Freundlich isotherm was fit to sorption data for river
gravel and limestone substrates (Sikora et al., 2000) They
reported n = 0.43 and KF = 22.6 for river gravel, and n = 0.43
and KF = 6.6 (see Equation 11.13)
Manganese is found in wetland plants, algae, and
sedi-ments Concentrations in sediments exposed to mine waters
may be very high, up to 10,000 µg/g For municipal
waste-water treatment wetlands, sediment manganese is typically
200–500 µg/g (Table 11.21) Manganese concentrations in
plant tissues are of the same order of magnitude, and
above-ground values do not differ much from belowabove-ground values
(Table 11.22)
The general conception is that in the aerobic, surface
waters of a wetland, oxidized forms are abundant, Mn(IV),
while in the anaerobic soils and sediments, reduced forms
prevail, Mn(II) (La Force et al., 2002) As a consequence,
both manganese forms in sediments and manganese cycling
are driven by redox patterns For example, at the Cataldo,
Idaho, mine drainage wetlands, winter represented aerobic
conditions, while spring had deeper waters and anaerobic
conditions in the sediments (La Force et al., 2002) As a
result, oxides were 34% of the total manganese in winter, but
only 3% in spring In general, the ratio of oxidized to reduced
manganese species was 1:1 in spring and 1:8 in winter
The storage of manganese in wetlands entails little or no risk
for waters other than acid mine drainage, because sediment
con-centration standards are typically quite high (see Table 11.21)
It is possible to estimate the sediment concentrations created
by sustainable removals of manganese, in terms of the dilution
of the manganese storage, by the accretion of new wetland
sol-ids For example, consider 200 dry g/m2·yr of new sediments,
originating from 1,000 dry g/m2·yr of biomass production
If the sediment concentration is to be kept below some limiting
level, such as the 40,000 µg/g severe effects level of the Ontario
guideline, for that Ontario guideline, deposition of 8 g Mn/m2·yr could be sustainably tolerated Meeting sediment standards on a sustainable basis is easily achieved for all concentrations
Performance of Wetlands for Manganese Removal
Manganese is typically removed in FWS wetlands (Table 11.23) For numerous systems, with inlet manganese ranging from 0.1–38,000 µg/L, the median concentration reduction
is 54% There is an increasing wetland exit concentration in response to increases in wetland manganese loading (Fig-ure 11.14) Outlet concentrations are below 1.0 mg/L for wetlands receiving leachates and other waters, but coal mine drainage wetlands are much more heavily loaded, and can have exit concentrations up to 20 mg/L
Horizontal subsurface constructed wetlands, where tion beds are usually anoxic or anaerobic, may release man-ganese over the period of operation This is due to dissolution
filtra-of manganese oxyhydroxides precipitates as a consequence
of low redox potential If redox conditions become very low and sulfate is present, manganous ions may precipitate with hydrogen sulfide from sulfate reduction to form insoluble sulfides Vymazal and Krása (2003) reported a substan-tial reduction of Mn in a HSSF constructed wetland in the Czech Republic; average inflow concentration of 278 μg/L was reduced to 53 μg/L However, results from three other HSSF systems in the Czech Republic exhibit substantial Mn release (Table 11.23) Vertical flow constructed wetlands due
to higher oxygenation of the bed exhibit good removal of manganese (Table 11.23)
There are two popular methods of interpreting performance data for metal removal in wetlands: the areal load removal and the first-order removal model These are both explored in detail for iron and manganese in a 35-wetland data set by Tarutis
TABLE 11.21
Manganese Content of Top Sediments in a Variety of Wetlands
Panel, Ontario Cattail marsh Urban stormwater 35 Goulet and Pick (2001)
Monahan, Ontario Cattail marsh Urban stormwater 50 Goulet and Pick (2001)
Falconbridge, Ontario Cattail marsh Acid mine drainage 15 Goulet and Pick (2001)
Riverwalk, Ontario Cattail marsh Tailings leachate 55 Goulet and Pick (2001)
West Page Swamp, Idaho Cattail, Arrowhead Tailings leachate 12,500 DeVolder et al (2003)
Widows Creek, Alabama Cattail, Juncus Tailings leachate 200–400 Ye et al (2001a,b)
Show Low, Arizona Pintail and telephone Municipal 521 NADB database (1998)
Tres Rios, Arizona Four wetlands Municipal 314 NADB database (1998)
Champion Paper, Florida Pilot Pulp and paper 285 NADB database (1998)
Sacramento, California Pilot Secondary 206–415 Nolte and Associates (1998b)
Leadville, Colorado Salix and Carex Mine water 9,500–1,790 August et al (2002)
Cataldo, Idaho Typha and Scirpus Mine water 1,600 Hansel et al (2002)
Monroe County, New York Phragmites FWS Landfill leachate 113 Eckhardt et al (1999)
Monroe County, New York Phragmites FWS Landfill leachate 303 Eckhardt et al (1999)
Keyser’s Ridge, Maryland Peat bed Highway runoff 236 Wieder et al (1988)
Lick Run, Ohio Mushroom compost Acid mine 395 Mitsch and Wise (1998)
Trang 34436 Treatment Wetlands
et al (1999) The former presumes a fixed removal per square
meter of wetland, regardless of inlet concentrations and flows,
and is basically a zero-order model The latter separately
includes the effects inlet concentration and flow rate
A problem of the zero-order model is that it cannot be
transferred from high loadings to low loadings The
recom-mended design removal rates are low: 0.5–1.0 g/m2·d (Hedin
et al., 1994); 0.5 g/m2·d (PIRAMID Consortium, 2003a)
However, this removal far exceeds the inlet loading to
non-mine water wetlands, which is only half that value at a
maxi-mum (Figure 11.14), and removal is not complete for those
lightly loaded systems
Miretsky et al (2004) determined first-order volumetric
rate constants for batch floating plant mesocosms For initial
concentrations of 1–4 mg/L, 87–98% of the manganese was
removed in less than one day for Pistia stratiotes Resulting
values of kV were 5.8 h−1 for Pistia stratiotes and 28.9 h−1 for
Spirodela intermedia Sikora et al (2000) also found very
high plug flow rate constants for SSF systems, with 10–60
m/yr in river gravel wetlands and 100–600 m/yr in limestone
wetlands Tarutis et al (1999) took data at 35 FWS coal mine
drainage wetlands over a one-year period Plug flow rate stants averaged 21 m/yr
con-Plants are a minor repository for removed manganese
The Ye et al (2001a) Widows Creek, Alabama, study mined that Typha latifolia and Juncus effusus contained
deter-just 0.95% of the annual amount of manganese entering the system Vymazal and Krása (2005) found 78% of the added manganese in sediments and belowground plant parts in a HSSF wetland treating domestic wastewater, and 1.73% in aboveground plant parts The majority of removed man-ganese is therefore associated with wetland sediments, in sorbed or chemically precipitated forms Long-term sustain-able removal requires continuing maintenance of oxidizing conditions
Example Treatment Wetlands for Manganese Removal
Quaking Houses, County Durham, United Kingdom (Younger et al., 2002)
Leachate from an abandoned colliery, containing up to 15 mg/L manganese and 30 mg/L of iron, was discharging into
TABLE 11.22
Manganese Content of Above- and Belowground Plant Parts in a Variety of Wetlands
Water (µg/L)
Above (µg/g)
Below (µg/g) Reference
TVA Mussel Shoals, Alabama SSF CW Scirpus acutus 100 19 23 Behrends et al (1996)
TVA Mussel Shoals, Alabama SSF CW Scirpus atovirens 100 10 17 Behrends et al (1996)
TVA Mussel Shoals, Alabama SSF CW Scirpus cyperinus 100 11 14 Behrends et al (1996)
TVA Mussel Shoals, Alabama SSF CW Phalaris arundinacea 100 20 48 Behrends et al (1996)
TVA Mussel Shoals, Alabama SSF CW Phragmites australis 100 28 62 Behrends et al (1996)
TVA Mussel Shoals, Alabama SSF CW Typha spp. 100 12 38 Behrends et al (1996)
Widows Creek, Alabama FWS CW Typha latifolia 7,600 1,097 200 Ye et al (2001a, b)
Coeur d’Alene, Idaho FWS Nat Typha latifolia — 1,300 — DeVolder et al (2003)
Nucice, Czech Republic SSF CW Phragmites australis 278 450 — Vymazal and Krása (2005)
Poland FWS Nat Phragmites australis 502 122 — Samecka-Cymerman and Kempers (2001) Nucice, Czech Republic SSF CW Phalaris arundinacaea 278 41 — Vymazal and Krása (2005)
Poland FWS Nat Phalaris arundinacea 898 619 — Samecka-Cymerman and Kempers (2001)
Widows Creek, Alabama FWS CW Juncus effusus 7,600 312 117 Ye et al (2001a, b)
Coeur d’Alene, Idaho FWS Nat Sagittaria latifolia — 830 — DeVolder et al (2003)
Bielkowo, Poland SSF CW Glyceria maxima — 241 545 Obarska-Pempkowiak et al (2005)
Bielkowo, Poland SSF CW Typha latifolia — 540 — Obarska-Pempkowiak et al (2005)
Bielkowo, Poland SSF CW Phragmites australis — 158 — Obarska-Pempkowiak et al (2005)
Chaco-Pampa, Argentina FWS FAP Pistia stratiotes 1,000 1,319 — Miretsky et al (2004)
Chaco-Pampa, Argentina FWS FAP Spirodela intermedia 1,000 5,038 — Miretsky et al (2004)
Cataldo, Idaho FWS Nat Typha latifolia 135 3,400 790 Hansel et al (2002)
Cataldo, Idaho FWS Nat Phalaris arundinacea 135 1,200 1,500 Hansel et al (2002)
Cataldo, Idaho FWS Nat Scirpus microcarpus 135 1,800 1,900 Hansel et al (2002)
Cataldo, Idaho FWS Nat Equisetum arvense 135 1,500 1,000 Hansel et al (2002)
Monroe County, New York FWS CW Phragmites australis — 265 567 Eckhardt et al (1999)
Note: FWS = free water surface; SSF = subsurface flow; CW = constructed wetland; Nat = natural wetland; FAP = floating aquatic plants.
Trang 35a stream (Stanley Burn), where it killed all aquatic life in its
path A 45-m2 pilot wetland was found to be effective,
com-prised of a shallow pond with a substrate of stable waste
(manure and straw) Subsequently, a full-scale, four-cell FWS
series wetland was implemented in 1997 The first two cells,
totaling 440 m2, were the heart of the system, with two
follow-on cells regarded as partly cosmetic The two working cells
contained baffles and islands to prevent short-circuiting The full-scale system substrate was a mixture of municipal com-post and manure The average hydraulic loading was about
20 cm/d The reduction in manganese was 26.4% over the first 27 months of operation, from 4.4 to 3.2 mg/L The areal removal rate was 0.26 g/m2·d (950 kg/ha·yr), and the first-order
areal removal rate constant was k = 22 m/yr (0.061 m/d).
TABLE 11.23
Removal of Manganese in Constructed Wetlands
Inlet (mg/L)
Outlet (mg/L)
Reduction (%)
Removal (g/m 2 ·yr) Reference FWS
35 systems Western Pennsylvania Coal mine water 10.0 8.4 16 266 Tarutis et al (1999)
10 systems TVA (Eastern United States) Coal acid mine 9.6 5.0 33 153 Brodie (1990)
124 systems Eastern United States Coal acid mine 37.7 24.0 34 — Wieder (1989)
Musselwhite Ontario Metal mine water 0.103 0.04 61 11.96 Bishay and Kadlec (2005)
6 Systems Champion, Florida Pulp and paper 0.600 0.318 47 5 NADB database (1998)
New Hanover County North Carolina Leachate 0.208 0.026 88 0.1 Unpublished data
Estevan Saskatchewan Municipal lagoon 0.113 0.175 55 -0.66 Unpublished data
HSSF
VF
Wapserveen 1 The Netherlands Municipal + dairy 0.22 0.02 91 0.11 Unpublished data
Trang 36438 Treatment Wetlands
#40 Gowen, Gaines Creek Watershed,
Oklahoma (Nairn, 2003)
Acid mine drainage, in the form of an artesian flow, was
add-ing unacceptable quantities of acidity, iron, and manganese
to Gaines Creek In 1998, the University of Oklahoma
con-structed a four-cell treatment wetland system to demonstrate
the ability of a passive system to treat this discharge The first
and third cells were vertical flow, with a layer of compost
above a limestone drainage layer (see Figure 11.15) The
sec-ond and fourth cells were horizontal aerobic units, and all were
planted with Typha latifolia A flow of 20 L/min (29 m3/d)
was directed to the wetlands, each of which had an area of
185 m2, resulting in a hydraulic loading of about 4 cm/d The
incoming water had pH = 3.4, Fe = 250 mg/L, Al = 36 mg/L,
and Mn = 14 mg/L At the system outlet, over the 8-month
study period, the pH was increased to 7.7, and Fe = 0.77 mg/L,
Al = 0.05 mg/L, and Mn = 5.8 mg/L The manganese load
removed was 3,796 kg/ha·yr (1.04 g/m2·d) Observations
dur-ing water quality sampldur-ing events indicated considerable
wildlife use of the treatment wetlands Several species of
amphibians (e.g., bullfrogs, leopard frogs, and salamanders),
reptiles (e.g., snapping turtles, garter snakes), birds (e.g., red winged blackbirds, killdeer, great blue herons), and mammals (e.g., moles, voles, coyotes) used the site Biological assess-ments in the summer of 2000 indicated healthy populations
of fish and macroinvertebrates in three of the four cells roinvertebrate community structure indicates a trend from tolerant to less tolerant species with flow through the wetland system In the final FWS cell, 314 bluegill fingerlings and
Mac-7 adults were seined (Nairn, 2003)
11.7 HEAVY METALS
C OPPER
Copper is an essential micronutrient for plants and animals because it is used for protein synthesis and in blood pigments Plants and animals require minimal amounts of this element, and deficiencies in nature are rare (Wetzel, 1983) The aver-age copper concentration in the world’s lakes and rivers is about 10 µg/L
Typically, copper is present in surface waters as chelated compounds of Cu(II) The ratio of free ionic to total dissolved
Flow out
Flow in
Organic material Limestone
Limestone
Flow out
Flow in
Organic material
Flow out
FIGURE 11.15 Three types of constructed wetlands used in acid mine drainage treatment.
Trang 37copper is often less than 1% and decreases with increasing
organic loads and pH above neutrality (Morel and Hering, 1993)
When chelated with organic compounds, copper may remain
relatively soluble Depending upon the nature of the
complex-ing ligand, the soluble complex may not be bioavailable
U.S EPA (2002a) sets criteria for freshwater
concentra-tions of copper according to hardness At hardness of 100
mg/L, the maximum concentration allowable is 13 µg/L, and
the continuous concentration allowable is 9 µg/L, as dissolved
copper U.S EPA (2002a) provides formulae for the limits at
other hardnesses, with soft waters having lower criteria The
maximum level for human ingestion is 0.61 mg/L
Sediment standards for copper have been set by the
Prov-ince of Ontario, and have been adopted in some of the states
in the United States These set a lowest effect level of 16 µg/g,
and a severe effects level of 110 µg/g (Persaud et al., 1993;
OMOEE, 1994) OMOEE (1994) has also identified the level
for presettlement deposits as 25 µg/g in Great Lakes
sedi-ments Wetzel (1983) reports sediments in Lake Schöhsee,
Germany, were 95 µg/g, at a water concentration of 1.0 µg/L
Copper is a biocide that is commonly used to control
algae and other organisms, such as schistosomes (swimmer’s
itch), which require snails and waterfowl as intermediate
hosts Copper has relatively low toxicity to benthic
macro-invertebrates and to fish, which may be unaffected to
con-centrations as high as 500 µg/L The sensitivity of algae and
the tolerance of fish and benthos to copper have resulted in
the widespread use of copper sulfate as an algaecide and
molluscicide in lakes
Wetland Processing and Storage of Copper
The storage of copper in wetlands entails a risk of creating
potentially impaired sediments It is possible to estimate the
sediment concentrations created by sustainable removals of
copper, in terms of the dilution of the copper storage by the
accretion of new wetland solids This is a mass balance on
the top layer of deposited material (Equation 11.22)
This analysis may be extended to estimate sediment
con-centrations For example, consider 200 dry g/m2·yr of new
sediments, originating from 1,000 dry g/m2·yr of biomass
production If the sediment concentration is to be kept below
some limiting level, such as the 110-µg/g severe effects level
of the Ontario guideline, Equation 11.22 can be solved for the
allowable removal flux For that Ontario guideline, deposition
of 22 mg Cu/m2·yr could be sustainably tolerated Meeting
rigorous sediment standards on a sustainable basis is not
eas-ily achieved for any but trace concentrations, but has been
accomplished for systems like Savannah River, South
Caro-lina But for high concentrations, like those entering White
Cedar Bog, Minnesota (620 µg/L), a plume of high sediment
concentration (100–3,000 µg/g) developed (Eger et al., 1980).
Copper is found in wetland plants, algae, and sediments
Concentrations in algal tissues are typically higher than in
plants and sediments, with concentrations of 100–1,000 µg/g
dry weight for a number of species (Vymazal, 1995) In
contrast, copper concentrations in plants are much lower,
approximately 1–20 µg/g dry mass (Table 11.24) However,
if the water concentration is increased to high levels, more
copper is accumulated (Qian et al., 1999; Manios et al.,
2003) Aboveground plant parts are of lowest concentration, and belowground organs are somewhat higher Wetland sedi-ments have the highest levels, and are therefore the major repository of stored copper
Copper Removal Processes
Constructed wetlands have the potential to trap and remove metals contained in wastewater Long-term removal is expected to occur by accumulation and burial in the plant detritus in a manner similar to the removal of phosphorus
Chemical Precipitation
Copper forms very insoluble compounds with sulfur, ing both cupric (Cu2+) and cuprous (Cu+) sulfides (Sobolewski, 1999):
Sulfide and bisulfide are formed by SRB in the anaerobic zones of treatment wetlands If a source of sulfate is pres-ent in the incoming water, the wetland can be configured to provide a sustainable supply of sulfide (Sobolewski, 1996) Copper also forms insoluble hydroxides and carbonates (Morel and Hering, 1993) However, they are not of impor-tance in the presence of the more insoluble sulfide
The removal of copper can also take place through precipitation with iron and manganese oxides However, this mechanism is contingent on considerable supplies of iron, which are typically present only in a fraction of cases Al- though iron and manganese oxides are generally excellent scavengers for other metals, they are unstable under anoxic
co-conditions (Knox et al., 2004).
where P represents the organic material (peat).
If Equation 11.38, cation exchange, is presumed to sent system performance, then the amount of copper bound
repre-is represented by (Kadlec and Keoleian, 1986)
where the bracket notation denotes molar concentration
This suggests that the partition coefficient ([CuP2]/[Cu2+] =
Trang 38440 Treatment Wetlands
TABLE 11.24
Copper Content of Wetland Plants and Sediments
Wetland Plant and Part Reference
Water (µg/L)
Solid (µg/g) Plant Shoots
Plant Roots
Plant Rhizomes
Sediments
Note: The corresponding water concentrations are approximate.
a Roots and rhizomes.
Trang 39CS/CL) should go down markedly with decreasing pH, which
is in fact the observation of many investigators, as shown in
Kadlec and Keoelian (1986) Because of the exponent of two
on hydrogen ion concentration in Equation 11.39, halving the
pH decreases the partition coefficient by a factor of 4 The
concentration of available exchange sites, [HP], is related to
the CEC of the peat Brown et al (2001) found that the
cop-per sorption potential of various peats was linearly correlated
with their CEC Uptake ranged from 10–60 mg/g to 100–200
meq/100 g (R2 = 0.90)
Equation 11.39 postulates that there are a finite number of
exchange sites, and hence the uptake of copper should reach a
maximum The Langmuir isotherm provides for such
satura-tion, and fits peat sorption data (Chen et al., 2001; see
Equa-tion 11.11)
The maximum capacity for copper is CSmax = K/a Brown
et al (2001) found capacities from 10–60 mg/g for 11 Irish
peats, whereas Chen et al (2001) found 13 mg/g for a New
Zealand peat Freundlich isotherms are also often used, and fit
nearly as well (Kadlec and Rathbun, 1984) (Equation 11.13)
Kadlec and Rathbun (1984) reported n = 0.4 and KF =
3.4 at pH = 6.5, and 2.0 at pH = 5.2 Chen et al (2001)
reported n = 0.145 and KF = 5.6 at 3.1 < pH < 3.6 Whichever
models are used, peats have the ability to store very large
quantities of copper By extrapolation, organic substrates in
general have similarly large capacities According to
Equa-tion 11.13, peats can store 5–10 mg/g for water concentraEqua-tions
of 1–10 mg Cu/L and circumneutral pH
Performance of Wetlands for Copper Removal
Copper is effectively removed in FWS wetlands (Table 11.25)
For 26 systems, with inlet copper ranging from 1 to 7,300
µg/L, the median concentration reduction is 66% There is a
possibility that first-order models of copper removal would
be appropriate (Tarutis et al., 1999), but there are no
cali-brations for existing systems It is probable that for overland
flow wetlands, the rate-limiting step is the transfer of
cop-per from the water to sorption and precipitation sites in the
sediments Traditional mass transfer modeling would utilize
a first-order model for that process (see Chapter 6) It is also
likely that percentage reductions in Table 11.25 would be
greater if the hydraulic efficiencies were higher, e.g., closer
to plug flow The Sinicrope et al (1992) data correspond
to plug flow k-values from 18 to 47 m/yr for a SSF system
Vymazal and Krása (2003) reported the k-values of 17 m/yr
and 15.5 m/yr for HSSF systems in Nucˇice and Morˇina, the
Czech Republic However, in the HSSF system at Brˇehov,
copper was washed out of the system This corresponds well
with increase concentrations of iron and manganese at the
outflow from this system The k-value for this system was
−5.8 m/yr Kadlec and Srinivasan (1995) report copper
uptake in FWS cattail microcosms of 25 < kPF < 120 m/yr
The Savannah River, South Carolina, results give a
first-order areal plug flow removal rate constant kPF y 75 m/yr
These are consistent with estimates of mass transfer
coef-ficients (Kadlec and Knight, 1996)
Quite complicated models have been written for copper removal The effort of Lung and Light (1996) was exercised, but not calibrated or verified The most significant effort was the development and calibration of the CWFATE model for the Sacramento, California, project (Jones & Stokes Associates, 1993; Nolte and Associates, 1998a,b) CWFATE attempts to describe water budgets, copper biomass cycles, and partitioning, but not chemical precipitation
Plants are a minor repository for removed copper The
Murray-Gulde et al (2005) Savannah River, South Carolina, study determined that Scirpus californicus took up 6.76%
of copper entering the system In the Sinicrope et al (1992)
study, the removed copper was found mostly in the soil (91%), with smaller amounts in fine roots (8%), and the bal-ance in coarse roots, rhizomes, and shoots Vymazal and Krása (2005) found 76% of the added copper in sediments and belowground plant parts in an HSSF wetland treating domestic wastewater, and 6.3% in aboveground plant parts.The majority of removed copper is therefore associated with wetland sediments, in sorbed or chemically precipitated forms These may be categorized according to sequential
extraction schemes (Morea et al., 1989; Sobolewski, 1996)
The principal forms are associated with iron and manganese oxides, sulfides, and exchange sites on organics (Figures 11.16 and 11.17) In each case, long-term sustainable removal requires a continuing supply of secondary materials
Anaerobic Wetlands
Many wetland systems have been constructed using post or other organic waste to generate an anaerobic envi-ronment and provide a source of organic carbon (Skousen,
com-1997; Younger et al., 2002; Eger and Wagner, 2003) (see
Figure 11.15) These wetlands include various flow patterns, including fully flooded VF downflow and shallow FWS over-land flow
Reduction of organic matter over sulfate generates gen sulfide (Equations 11.1 and 11.2), which may react with copper to form insoluble copper sulfides (Equations 11.35 and 11.36) Lifetime estimates based on the total amount of carbon in these systems suggested that the substrate would last for several decades, but data indicate that these predic-tions were overly optimistic Eger and Wagner (2003) suggest that the amount of available substrate carbon is about 10%
hydro-of the theoretical Decaying wetland plants are a potential carbon source Bioavailable carbon production in wetlands is about 60 g C/m2·yr (see the denitrification section of Chapter 9) According to Equation 11.2, this would support sulfide production of 80 g S/m2·yr, a factor of 50 less than the typical
design rate recommended by Wildeman et al (1993b) The
corresponding copper removal rate is 160 g Cu/m2·yr, which
is also far less than the design value of 3,650 g Cu/m2·yr tentatively advanced by the PIRAMID Project of the Euro-pean Union (PIRAMID Consortium, 2003a) for anaerobic wetlands Results from HSSF wetlands (Table 11.25) indi-cate generally high removal of copper (81–84%), but in one instance copper was released from the system