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36 Aeronautical Engineer’s Data Book Square matrix This is a matrix having the same number of rows and columns.. Diagonal matrix This is a square matrix in which all the elements are z

Trang 1

�+

3

33 33 33

� �

31 Fundamental dimensions and units

33 (A 2 B) = A 2 33 + 33 2 B

= – 33 (B 2 A)

dt Gradient

The gradient (grad) of a scalar field +(x, y, z) is

i 33 + j 33 + k 3

� ∂

grad + = 6+ =

j

3 3

i +

∂ 3

=

= V x (x, y, z) i + V y (x, y, z) j + Vz

∂ +

3 3

∂ +

3 3

div = 6· 3Vx Vy V

∂x ∂y ∂z

Curl

Curl (rotation) is:

z

curl V = 6 2 V = ∂ ∂ ∂

Vx Vy Vz

3 3

3 Vz V

∂y ∂z

3 3

3 Vx V

∂z ∂x

=

3 3

3 Vy V

∂x ∂y k

x +

2.8.8 Differentiation

Rules for differentiation: y, u and v are

functions of x; a, b, c and n are constants

33 (au ± bv) = a 33 ± b 33

33 = u 33 + v 33

33 33 = 33 33 – 33 33

Trang 2

3 3

3

3

3

d

3

x

3

d (u

n ) = nu n–1 u

d3

x

d

x

du

3

d

3

u

n

3

x

3

u

= –

n

= 1/ ,

x

3

3

d

3

x

d

3 if 3dx3

d ≠ 0

u

d

3

x

3

d

u

f (u) = f’(u)

d3

x

d

3

x

d

3

x

3

d a f(t)dt = f(x)

b

d

3

x

3

d x f(t)dt = – f(x)

b

f(x, t)dt = b

f

3

∂x

d

3

x

3

v

f(x, t)dt = u

3

x

d

3

f

3 dt + f (x, v)

d

3

x

3

u

3

x

d

3

– f (x, u)

d Higher derivatives

d

3 2 y

dx2

d

3

x

d

3

y

Second derivatives = 3

x

3

d

= f"(x) = y"

3 2

dx2

d

3

x

d

3

d �2

+ f '(u)

3

d 3 f(u) = f "(u)2

x

Derivatives of exponentials and logarithms

d

(ax + b) n = na(ax + b) n–1

3

x

3

d

d

3

x

3

d e

ax = ae ax

d

3

x

3

d ln ax = 3

x

1

3 , ax > 0

Trang 3

3

33 Fundamental dimensions and units

d

3

x

3

d a

u = a u ln a u

d3

x

d

3

d3

x

d

3 3

x

3

d loga u = log a e

1 3

u

Derivatives of trigonometric functions in radians

sin x = cos x, cos x = – sin x

3

x

3

x

3

d

d

3

x

3

d tan x = sec

2 x = 1 + tan2 x

d

3

x

3

d cot x = –cosec

2x

3

x

3

x

3

c

sec x = 2

os = sec x tan x

3

x

3

x

3

s

cosec x = –

in2 = – cosec x cot x

arcsin x = –

3

x

3

x

3

d arccos x

1

= 33 for angles in the(1 – x2)1/2 first quadrant

Derivatives of hyperbolic functions

sinh x = cosh x, cosh x = sinh x

3

x

3

x

3

d

tanh x = sech2 cosh x = – cosech2 3

x

3

x

3

d

(arcsinh x) = 32 +1)1/2

3

x

3

(arccosh x) = 3

1)1/2

3

x

3

x

Trang 4

3

x

Partial derivatives Let f(x, y) be a function of

the two variables x and y The partial deriva­ tive of f with respect to x, keeping y constant is:

f (x + h, y) – f (x, y)

Similarly the partial derivative of f with respect

to y, keeping x constant, is

f

3

∂ 3 3

v

3

∂y k→0

Chain rule for partial derivatives To change

variables from (x, y) to (u, v) where u = u(x, y),

v = v(x, y), both x = x(u, v) and y(u, v) exist and f(x, y) = f [x(u, v), y(u, v)] = F(u, v)

f

3

3

u

3

3 = 3

f (x, y + k) – f (x, y)

f

3

3

f

3 y

∂v ∂v ∂v ∂y

f

3

y

3

f

x

∂u ∂x ∂u ∂y

f

3

∂x 3x

3 u

∂ 3 3

x

∂ 3

3 ∂ F + ∂ ∂ , v F ∂y ∂ 3f 3y

3 u

∂ 3 3

y

∂ 3

3 F + v F

∂ ∂ ∂

2.8.9 Integration

a+1

x

a ≠ –1

1

3

a

e

3

+

kx

k

,

kx

e

a x

a > 0, a ≠ 1

a

3

ln ,

ln x x ln x – x

tan x ln | sec x |

cot x ln | sin x |

sec x ln | sec x + tan x |

3 1 3

tan 3 (x + 3 π) |

Trang 5

33

33

2

35 Fundamental dimensions and units

3 2 1

3 x |

ln | tan

cosec x

sin2x 323(x – sin 2x)323

2 3213(x + sin 2x)3213

cos x

sec2 x tan x

sinh x cosh x

cosh x sinh x

tanh x ln cosh x

sech x 2 arctan e x

3 2 1 3

cosech x ln | tanh x |

sech2 x tanh x

3a2+ x

1

a

1

a

x

3 , a ≠ 0

arctan

1 a – x

�– 3 ln a ≠ a

a

3

x

3

a + ,

x – a

32

3

a

1

a ≠ 0

a

3

x +

3

a

3

a ≠ 0 arcsin

2)1/2

|

3

| a ,

ln [x + (x2 – a2)1/2]

1

2)1/2

a

x

3 , a ≠ 0

arccosh

2.8.10 Matrices

A matrix which has an array of m 2 n numbers arranged in m rows and n columns is called an

m 2 n matrix It is denoted by:

a11 a12 a 1n

a

a21 a22

a m1 a m2 a mn

Trang 6

36 Aeronautical Engineer’s Data Book

Square matrix

This is a matrix having the same number of rows and columns

a11 a12 a13

a21 a22 a23 is a square matrix of order 3 2

a31 a32 a33 3

Diagonal matrix

This is a square matrix in which all the elements are zero except those in the leading diagonal

a11 0 0

0�

0 a22 is a diagonal matrix of order 3

0 0 a33 2 3

Unit matrix

This is a diagonal matrix with the elements in the leading diagonal all equal to 1 All other elements are 0 The unit matrix is denoted

by I

1 0 0

0 1 0

I = � �0 0 1

Addition of matrices

Two matrices may be added provided that they are of the same order This is done by adding the corresponding elements in each matrix

a11 a12 a13�+ b11 b12 b

a21 a22 a23 �b21 b22 b23

a11 + b11 a12 + b12 a13 + b

= �a21 + b21 a22 + b22 a23 + b23

Subtraction of matrices

Subtraction is done in a similar way to addition except that the corresponding elements are subtracted

a11 a12 b11 b12 a11 – b11 a12 –b12

� �a21 a22 – � �b21 b22 = �a21 –b21 a22 –b22�

Trang 7

� � � �

37 Fundamental dimensions and units

Scalar multiplication

A matrix may be multiplied by a number as follows:

a11 a12 ba11 ba12

b� �a21 a22 = �ba21 ba22�

General matrix multiplication

Two matrices can be multiplied together provided the number of columns in the first matrix is equal to the number of rows in the second matrix

b11 b12

a11 a12 a13

b21 b22

a21 a22a23

b31 b32

a11b11+a12b22 +a13b31 a11b12 +a12b22 +a13b32

= �a21b11 +a22b21 +a23b31 a21b12 +a22b22 +a23b32�

If matrix A is of order (p 2 q) and matrix B is

of order (q 2 r) then if C = AB, the order of C

is (p 2 r)

Transposition of a matrix

When the rows of a matrix are interchanged

with its columns the matrix is said to be trans­

posed If the original matrix is denoted by A, its

transpose is denoted by A' or A T

a11 a12 a13

then A T = � �

a

21 a22a

a13 a23 Adjoint of a matrix

If A =[a ij ] is any matrix and A ij is the cofactor

of a ij the matrix [A ij]T is called the adjoint of A

Thus:

a

a

21 a22 a 2n A12 A22 A n2

11 a12 a 1n

adj A = �A11 A21 A n1

A =

a n1 a n2 a mn A1n A2n A nn

Trang 8

Singular matrix

A square matrix is singular if the determinant

of its coefficients is zero

If A is a non-singular matrix of order (n then its inverse is denoted by A–1 such that AA

= I = A–1 A

adj (A)

A–1 = 33 ∆ = det (A)

A ij = cofactor of a ij

a

a11 a12 a 1n

� �A11 A21 A n1

21 a22 a 2n A12 A22 A n2

A–1 = 31 3 . .

If A = � ∆

a

n1 a n2 a nn A 1n A 2n A nn

2.8.11 Solutions of simultaneous linear equations

The set of linear equations

a11x1+ a12x2 + + a 1n x n = b1

a21x1+ a22x2 + + a 2n x n = b2

a n1 x1+ a n2 x2 + + a nn x n = b n

a

where the as and bs are known, may be repre­ sented by the single matrix equation Ax = b, where A is the (n 2 n) matrix of coefficients,

ij , and x and b are (n 2 1) column vectors

The solution to this matrix equation, if A is non-singular, may be written as x = A–1b

which leads to a solution given by Cramer’s

rule:

x i = det D i /det A i = 1, 2, , n

where det D i is the determinant obtained from

det A by replacing the elements of a ki of the ith column by the elements b k (k = 1, 2, , n) Note that this rule is obtained by using A–1 = (det A)–1

adj A and so again is of practical use only when

n ≤ 4

Trang 9

+ +

x

39 Fundamental dimensions and units

If det A = 0 but det D i ≠ 0 for some i then the equations are inconsistent: for example, x + y =

2, x + y = 3 has no solution

2.8.12 Ordinary differential equations

A differential equation is a relation between a

function and its derivatives The order of the

highest derivative appearing is the order of the

differential equation Equations involving

only one independent variable are ordinary

differential equations, whereas those involv­

ing more than one are partial differential

equations

If the equation involves no products of the function with its derivatives or itself nor of

derivatives with each other, then it is linear Otherwise it is non-linear

A linear differential equation of order n has

the form:

d n–1

3

x

d

3 3

1

3

d

where P i (i = 0, 1 ., n) F may be functions of

x or constants, and P0 ≠ 0

First order differential equations

3 n

d

3 n

P0 y

dx + P1 + + P n–1 + P n y = F

3

y

d

3

d = f 3

x

y

x

y

3 homo- substitute u =

dy

3 )

3

g

geneous

(y

3

x

d

3y = f(x)g(y) separable

note that roots of

g(y) = 0 are also

solutions

3∂ 3∂ ∂

y

3

x

d

3

+ f(x, y) = 0 exact = g

and solve these

3

x

3g

= ∂

equations for +

+ (x, y) = constant

is the solution

f

3

y

and3

Trang 10

40 Aeronautical Engineer’s Data Book

dy

3

dx 3 + f(x)y linear Multiply through by

p(x) = exp(x f(t)dt)

p(x)y = x g(s)p(s)ds

+ C

Second order (linear) equations

These are of the form:

P0(x) 33 + P1 (x) 33 + P2 (x)y = F(x)

When P0, P1, P2 are constants and f(x) = 0, the

solution is found from the roots of the auxiliary equation:

P0m2+ P1m + P2= 0

There are three other cases:

(i) Roots m =  and  are real and  ≠ 

y(x) = Ae x + Be x

(ii) Double roots:  = 

x

y(x) = (A + Bx)e

(iii) Roots are complex: m = k ± il

y(x) = (A cos lx + B sin lx)e kx

2.8.13 Laplace transforms

If f(t) is defined for all t in 0 ≤ t < ∞, then

L[f(t)] = F(s) = �∞

e –st f(t)dt

0

is called the Laplace transform of f(t) The two functions of f(t), F(s) are known as a transform

pair, and

f(t) = L–1[F(s)]

is called the inverse transform of F(s)

c1f(t) + c2g(t) c1F(s) + c2G(s)

Trang 11

33

33

33

33

t

0

(–t) n f(t)

n

s n

d

F

3

d

3

e at f(t)

e

F(s – a) –as F(s) f(t – a)H(t – a)

n

t n

d

f

3

d

3

3

a

1

3 e –bt sin at, a > 0

n

s n F(s) – s n–r f (r–1) (0+)

r=1

1 2

(s = b)2 + a

s + b –bt

(s + b )2 + a

1

3

a

1

3 e –bt sinh at, a > 0

(s + b)2 + a2

s + b

2

(πt)–1/2

n t n–1/2

s

(s + b)2 + a

–1/2

s –(n+1/2)

33,

1·3·5 (2n –1)�π

2

p(– t)

1/2

2(π 3)

4

ex a

(a > 0) e –a� s

t

2.8.14 Basic trigonometry

Definitions (see Figure 2.9)

sine: sin A = 3

r

y

3 cosine: cos A = 3

r

x

3

3

x

y

3 cotangent: cot A = 3

y

x

3

tangent: tan A =

r 33

y

secant: sec A = cosecant: cosec A =

Trang 12

7 3

A

y

r

x

Fig 2.9 Basic trigonometry

Relations between trigonometric functions

sin2 A + cos2 A = 1 sec2 A = 1 + tan2 A

cosec2 A = 1 + cot2 A

sin A = s cos A = c tan A = t

sin A s (1 – c2)1/2 t(1 + t2)–1/2

cos A (1 – s2)1/2 c (1 + t2)–1/2

tan A s(1 – s2)1/2 (1 – c2)1/2/c t

A is assumed to be in the first quadrant; signs

of square roots must be chosen appropriately in other quadrants

Addition formulae

sin(A ± B) = sin A cos B ± cos A sin B cos(A ± B) = cos A cos B 7 sin A sin B

tan A ± tan B tan(A ± B) = 3

tan A tan B

Sum and difference formulae

3 2 1

sin A + sin B = 2 sin (A + B) cos (A – B)

3 2 1

sin A – sin B = 2 cos (A + B) sin (A – B)

3 2 1

cos A + cos B = 2 cos (A + B) cos (A – B)

3 1

cos A – cos B = 2 sin (A + B) sin (B – A)

Trang 13

43 Fundamental dimensions and units

Product formulae

3 2 3

sin A sin B = {cos(A – B) – cos(A + B)}

3 2 1 3

cos A cos B = {cos(A – B) + cos(A + B)} sin A cos B =323{sin(A – B) + sin(A + B)}

Powers of trigonometric functions

sin2 A =3213– 3213cos 2A

2 A =3213 3213 cos 2A

cos

sin3 A =3433sin A – sin 3A 3413

3 A =3433cos A +3413cos 3A

cos

2.8.15 Co-ordinate geometry

Straight-line

General equation

ax + by + c = 0

m = gradient

c = intercept on the y-axis

Gradient equation

y = mx + c

Intercept equation

x

3

A 3y3

B

A = intercept on the x-axis

= 1

B = intercept on the y-axis

Perpendicular equation

x cos  + y sin  = p

p = length of perpendicular from the origin to the line

 = angle that the perpendicular makes

with the x-axis

The distance between two points P(x1, y1) and

Q(x2, y2) and is given by:

�2)2 + (�)2

PQ = (x1– xy1– y2�

The equation of the line joining two points (x1,

y1) and (x2, y2) is given by:

3

3

y

y – y1

– y

x – x

3

3

x

1

=

– x

Trang 14

Circle

General equation x2– y2+ 2gx + 2fy + c = 0 The centre has co-ordinates (–g, –f)

The radius is r = g�2+ f 2–c

The equation of the tangent at (x1, y1)

to the circle is:

xx1+ yy1+ g(x + x 1 ) + f(y + y 1 ) + c = 0

The length of the tangent from to the circle is:

t2= x1+ y1+ 2gx1+ 2fy1+ c

Parabola (see Figure 2.10)

SP

Eccentricity = e = 33 = 1

PD

With focus S(a, 0) the equation of a parabola

is y2= 4ax

The parametric form of the equation is x =

at2, y = 2at

The equation of the tangent at (x1, y1) is yy1

= 2a(x + x1)

Ellipse (see Figure 2.11)

SP

Eccentricity e = 33 < 1

The equation of an ellipse is 33 + 33 = 1a2 b

where b2= a2 (1 – e2

The equation of the tangent at (x1, y1) is

33 + 33 = 1

a2 b2

The parametric form of the equation of an

ellipse is x = a cos , y = b sin, where  is

the eccentric angle

Hyperbola (see Figure 2.12)

SP

Eccentricity e = 33 > 1

The equation of a hyperbola is 33 – 33 = 1a2 b

where b2= a2(e2

Trang 15

45 Fundamental dimensions and units

y axis

Focus S(a,0)

x axis

Fig 2.10 Parabola

D P

S(ae,0)

b

b

a a

x axis

y axis

Fig 2.11 Ellipse

y axis

a a

x axis

D

S

P S(ae,0)

Fig 2.12 Hyperbola

Trang 16

46 Aeronautical Engineer’s Data Book

The parametric form of the equation is x =

a sec , y = b tan where  s the eccenteric

angle

The equation of the tangent at (x1, y1) is

xx1 yy1

33 – 33 = 1

a2 b2

Sine Wave (see Figure 2.13)

y = a sin(bx + c)

y = a cos(bx + c') = a sin(bx + c) (where c = c'+

where a = m2+ n, c = tan–1 (n/m)

y axis

x axis c/b

a

2 π/b

0

Fig 2.13 Sine wave

Helix (see Figure 2.14)

A helix is a curve generated by a point moving

on a cylinder with the distance it transverses parallel to the axis of the cylinder being proportional to the angle of rotation about the axis:

x = a cos 

y = a sin 

z = k

where a = radius of cylinder, 2 πk = pitch

Trang 17

47 Fundamental dimensions and units

a

z

y

x

Fig 2.14 Helix

2.9 Useful references and standards

For links to ‘The Reference Desk’ – a website containing over 6000 on-line units conversions

‘calculators’ – go to: www.flinthills.com/

~ramsdale/EngZone/refer.htm

United States Metric Association, go to: http://lamar.colostate.edu/~hillger/ This site contains links to over 20 units-related sites For guidance on correct units usage go to: http://lamar.colostate.edu/~hillger/correct.htm

Standards

1 ASTM/IEEE SI 10: 1997: Use of the SI

system of units (replaces ASTM E380 and

IEEE 268)

2 Taylor, B.N Guide for the use of the Inter­

national System of units (SI): 1995 NIST

special publication No 8111

Trang 18

48 Aeronautical Engineer’s Data Book

3 Federal Standard 376B: 1993: Preferred

Metric Units for general use by the Federal Government General Services Administra­

tion, Washington DC, 20406

Trang 19

Section 3

Symbols and notations

3.1 Parameters and constants

See Table 3.1

Table 3.1 Important parameters and constants

Planck’s constant (h)

Universal gas constant (R)

Stefan–Boltzmann constant ( )

Acceleration due to gravity (g)

Absolute zero

Volume of 1 kg mol of ideal

gas at 1 atm, 0°C

Avagadro’s number (N)

Speed of sound at sea level (a0)

Air pressure at sea level (p0)

6.6260755  10 –34 J s 8.314510 J/mol/K 5.67051  10 –8 W/m 2 K 4

9.80665 m/s 2

(32.17405 ft/s 2 ) –273.16°C (–459.688°F) 22.41 m 3

6.023  10 26 /kg mol 340.29 m/s (1116.44 ft/sec)

760 mmHg

= 1.01325  10 5 N/m 2

= 2116.22 lb/ft 2

Air temperature at sea level (T0

Air density at sea level (  0 ) 1.22492 kg/m 3

slug/ft 3 ) Air dynamic viscosity at sea 1.4607  10 –5 m 2 /s

3.2 Weights of gases

See Table 3.2

Table 3.2 Weights of gases

Gas kg/m 3 lb/ft 3

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