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UNCLASSIFIED AD 292177 kefmduced luf, Ute ARMED SERVICES TECHNICAL INFORMATION AGENCY ARLINGTON HALL STATION ARLINGTON 12, VIRGINIA UNCLASSIFIED

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UNCLASSIFIED

AD 292177 kefmduced

luf, Ute

ARMED SERVICES TECHNICAL INFORMATION AGENCY ARLINGTON HALL STATION ARLINGTON 12, VIRGINIA

UNCLASSIFIED

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NOTICE: When government or other dravings, speci- fications or other data are used for any purpose other than in connection with a definitely related government procurement operation, the U. S. Government thereby incurs no responsibility, nor any obligation whatsoever; and the fact that the Govern- ment may have fonnulated, furnished, or in any way supplied the said drawings, specifications, or other data is not to be regarded by implication or other- wise as in any manner licensing the holder or any other person or corporation, or conveying any rights or permission to manufacture, use or sell any patented invention that may in any way be related thereto.

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(;'S-2 -/

H

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4P $>

.^S ^ 'i

OQ

■ s AIR UNIVERSITY

UNITED STATES AIR FORCE

SCHOOL OF ENGINEERING

WRIGHT-PATTERSON AIR FORCE BASE, OHIO AST! A

AF-WP-O-MAY 62 3,500

J lj L, j \^.J

nsiA C

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TH3 EQUATIONS OF FLUID MECHANICS

HXPRESSED IN CURVILINEAR COORDINATES

GAE/ME/62-4

Bradley Sutter

Cant USAF

AF-W^-O-SEP 62 25

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THE EQUATIONS OF FLUID MECHANICS

EXPRESSED IN CURVILINEAR COORDINATES

THESIS

Presented to the Faculty of the School of Engineering of

the Air Force Institute of Technology

Air University

in Partial Fulfillment of the

Requirements for the Degree of

Master of Science

By

Bradley Sutter, B.S.

Capt USAF

Graduate Aeronautical Engineering

August 1962

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GA2/M3/62-4

Preface

In this thesis the methods of tensor analysis have

been used to obtain expressions for the basic equations

of fluid mechanics in terms of several orthogonal curvi-

linear coordinate systems. V/hile these methods can be

used with any valid coordinate transformations, the

reader should be cautioned that the specific results

obtained here are applicable only to the particular

transformations which are listed in Appendix A, There

are other methods of defining the various coordinate sys-

tems, but, to make use of these differing definitions,

the reader would have to start with the basic equations

listed in this report and derive his own final results.

It should also be emphasized that this report does

not attempt to explain the mechanics of tensor analysis.

If the reader is unfamiliar with this branch of mathematics

and wishes to gain the background to enable him to fill in

the steps which have been omitted in the development of the

relationships used in this report, the book by Sokolnlkoff

(Ref 4) Is an excellent text.

11

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GAE/Mß/62-4

The author wishes to express his gratitude to Lt.

Ray M. Bowen of the Mechanical engineering Department of

the Institute for the extensive help ho has given In the

preparation of this thesis. Lt. Bowen Is responsible for

giving the author his first appreciation of the powers of

tensor analysis, and for guiding him through the confusion

which occurred from time to time. If .here are any errors

remaining in this thesis, they are the author's and are

not due to any misinformation from Lt, Bowen.

Bradley Sutter

Hi

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GAE/ME/62-4

Contents

Page

Preface 11

List of Symbols vll

Abstract vlll

I. Introduction 1

II. The Basic Equations 3

Continuity Equation 3

Energy Equation 4

Equation of Motion 5

III. The Completed Transformations 9

Cartesian Coordinates 9

Continuity Equation 9

Energy Equation 9

Equation of Motion 11

Cylindrical Coordinates 12

Continuity Equation 12

Energy Equation 13

Equation of Motion 15

Spherical Coordinates 16

Continuity Equation 16

Energy Equation 17

Equation of Motion 19

iv

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GAE/ME/62-4

Contents

Page

Parabolic Coordinates 20

Continuity Equation 21

Energy Equation 21

Equation of Motion 24

Prolate Spheroidal Coordinates 25

Continuity Equation 26

Energy Equation 26

Equation of Motion 29

Spheroidal Coordinates 32

Continuity Equation 32

Energy Equation 32

Equation of Motion 36

Parabolic Cylinder Coordinates 38

Continuity Equation 3S

Energy Equation 39

Equation of Motion 4l

Elliptic Cylinder Coordinates 42

Continuity Equation 43

Energy Equation 43

Equation of Motion 45

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GAE/ME/62-4

Contents

Page

Ellipsoidal Coordinates 4?

Continuity Equation 4?

Energy Equation 48

Equation of Motion 5-

Confocal Parabolic Coordinates 56

Continuity Equation 57

Energy Equation 57

Equation of Motion 6l

Conical Coordinates 65

Continuity Equation 66

Energy Equation 66

Equation of Motion 70

IV. Conclusions 73

Bibliography 74

Appendix A: Description of Coordinate Systems .... 75

Appendix B: Derivation of Basic Equations

of Fluid Mechanics 87

Appendix C: The Three Basic Equations

(Gate-Fold) 94

Vita 96

vl

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3 i

GAE/M3/62-4

List of Symbols

P density

W tensor component of the velocity

Vt physical component of the velocity

Qij metric tensor, S^i ^ 0 • 6 ^ J

determinant of the metric tensor

time

^ Internal energy per unit mass

n enthalpy per unit mass

^ stress tensor, (= 'p^ + h"1*)

p pressure

viscous stress tensor

physical component of the viscous stress tensor

tensor component of the body force

• t physical component of the body force

Q, tensor component of the heat flux vector

4£' physical component of the heat flux vector

7 tensor component of the acceleration vector

JV physical component of the acceleration vector

tf coefficient of bulk viscosity

^T coefficient of shear viscosity

Where tensor quantities are defined, the symbols are the

same for covarlant or contravarlant tensors.

vll

F1

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GAE/Mii/62-il

Abstract

The applied science of fluid mechanics makes use of

three basic equations to analyze and predict the state of

a fluid In motion. These equations are the equations of

motion, energy, and continuity. In most flow problems,

these equations cannot be solved, or are very difficult

to solve, unless they are expressed in terms of a coordi-

nate system which conforms to the surface of the duct or

body which shapes the flow.

This report utilizes the methods of tensor analysis

to transform the basic equations from their Cartesian forms

to expressions in ten orthogonal curvilinear coordinate

systems. The derivation process is outlined, and the final

results are tabulated for each of the coordinate systems.

Although this report assumes a Newtonian fluid model, the

viscous stress components are listed separately so that,

given the proper expressions for the viscous stress com-

ponents, the results may also be applied to a non-Newton-

ian fluid.

vlil

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GAE/ME/62-4

THE EQUATIONS OF FLUID MECHANICS

EXPRESSED IN CURVILINEAR COORDINATES

I. Introduction

Fluid mechanics Is defined as the applied Science

which deals with the principles of both gaseous and liquid

flow. Practically, we are concerned with fluid flow over

solid bodies or through various types of ducts or channels.

In order to predict and describe such flow, we make use of

three basic equations: the continuity equation, the energy

equation, and the equation of motion. These equations are

dependent upon the use of some three-dimensional coordinate

system to describe the properties and the movement of a

fluid.

For simple flow patterns, such as flow over a flat

plate, rectangular Cartesian coordinates are adequate for

complete description of the flow characteristics. However,

for flow around more complex body shapes, we find that the

equations cannot be solved, or are extremely difficult to

solve, unless they are expressed in terms of a coordinate

system which is compatible with the geometry of the body.

In particular we must have a coordinate system which has

a coordinate surface closely approximating the shape of

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GAE/ME/62-4

the body. This is especially Important in enabling one

to express the boundary conditions in a simple form. Some

examples of flow situations which require more sophisti-

cated coordinate systems are: flow over submarine hulls,

whose shapes are elongated spheroids; flow through ellip-

tical pipes; and flow through converging-diverging nozzles,

in which the nozzle walls approximate hyperbololds of one

sheet.

The problem is one of expressing the familiar Cartes-

ian forms of the basic equations in terms of the various

curvilinear coordinate systems. To do this, the methods

of tensor analysis will be used. The general approach has

been outlined for the continuity and motion equations by

McConnell (Ref 1: 271-313), among others, and results have

been obtained for cylindrical and spherical coordinates.

The methods used in this report differ only slightly from

those used by McConnell.

The fluid model is assumed to be viscous, heat conduc-

ting, and isotroplc. Chemical, electromagnetic, radiation,

and diffusion effects are ignored. The fluid is also

assumed to be Newtonian. However, the expressions for the

viscous stress tensor are listed separately so that, given

the proper expressions for the viscous stress tensor, the

results may also be applied to non-Newtonian fluids.

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GAE/ME/62-4

II. The Basic aquations

The basic equations are presented here in fairly con-

ventional form, and they are then adapted to a form more

suitable for final tabulation. If the reader is interested

in the derivation of the equations, he is referred to

Appendix B.

Continuity Equation

The continuity equation can be expressed in tensor

notation as

af + (ftf1),. '- o , (i)

where t/'is the i'th component of the velocity vector, and

P is the density. The second term represents the diverg-

ence of a vector, and it can be expressed more conveniently

by using

(pi/0., = 7f ax'l/^ fv<j ) (2)

where V- represents the physical component of the velocity

vector. Substituting equation (2) into equation (l), we

obtain the continuity equation in its final 'form:

^ '/f ^'l/pS P') = 0 • (3)

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GAE/ME/62-4

Energy Equation

In tensor notation, one form of the energy equation Is

(vc^).^ f^Fl-%> i i (4)

where h Is enthalpy, fo',, Is the Ij'th component of the

viscous stress tensor, p Is pressure, and 0 is the i'th

component of the heat flux vector. By substituting physi-

cal components and making use of the general form of equa-

tion (2), we obtain the energy equation in Its final form:

-1-2./ /S' u £i:\ 1/ P -i 5 / /T - \ (5)

whore IT , F^ , and 9,; are the physical components of the

viscous stress tensor, the body force, and the heat flux

vector, respectively. The Ij'th component of the viscous

stress tensor can be written, after Sokolnlkoff (Ref 4:

321-324), as

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GA2AB/62-4

^■tg y.H,+ g tr^J , (6)

where n Is the coefficient of bulk viscosity (usually

taken to be zero), and ^T is the coefficient of shear vis-

cosity. After carrying out the indicated operations and

substituting the physical components for the velocity

vectors, we obtain

^ aP(9 3 ^3 9 i^J • (7)

V/e can obtain the physical components of 7TlJby multiplying

equation (7) by ffiu^faup . Although the multiplication will

not be shown here, the physical components, rather than the

tensor components, will be tabulated In the next section.

Equation of Motion

The tensor form of the equation of motion Is

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GAE/Ma/62-4

f(Wi)--3iKV , (8)

where ii is the i'th component of the acceleration vector,

and fij represents the viscous and pressure forces as

follows:

The physical component of the acceleration vector is

Tj r / ga><" Tfo= J($ÜHü Id) > (10)

and the physical component of the body force is

(11)

where Tt- and F,- represent the physical component of the

acceleration vector and the body force, respectively. By

substituting equations (10) and (11) into equation (9),

we obtain

f (^ " M = 7pS ^oj,^ (12)

which is the final form of the equation of motion.

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GAE/MH/62-4

The i'ih component of the acceleration vector Is

r I I ^■' i 1 (13)

The final form of the acceleration vector is obtained by

expanding equation (13) and substituting the physical com-

ponents of the velocity vectors:

r ^ j f aVi

^lax^^^Vj-^x^^Viljj . (i4)

The term on the right side of equation (12) can be ex-

panded, using equation (9), as follows:

1 ik v i / ^ ik v

where

(16)

Expanding equation (l6) to eliminate the Christoffel sym-

7

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GAE/ME/62-4

bols, we obtain, after simplifying

i 9 SM ^\* - i^lAq%tT^)

i 3 I M [<\i*) tr* . (i7)

Substituting equation (17) into equation (15), we obtain

I $&' b" J , da)

Substitution of the physical components of the viscous

stress tensor yields

all v - -i- [ n Xi? /JUilii-, ^4K\

1 - 9jiK xiiui (19)

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0AE/W62-4

III. The Completed Transformations

For convonioncc, the equations that are to be expres-

sed In the various coordinate systems have been restated

on a fold-out sheet in Appendix C.

Cartesian Coordinates

x = x xN 4 x'-- I (20)

'Ju- \~ - 3 33 i (21)

Continuity Equation.

M -^(f^VaVp^^l^fV.) - o (22)

Energy Equation. The left side of equation (5)

becomes

v.MMxt/M^v;)]! . (23,

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GAB/toE/62-i*

The remalnin? terms of interest arc

/M^/few^) =Ä(^^-.^-. ^tr*') + ^(v.fr'^V^" f V^^) +

?A^X* tv^ + v^") l (24)

3>K£ - ^ (v;p>tV5/? f vJt) > (25)

and

3 /^ f §c.^ 5#f) = f'P'm^&p. (26)

The components of the viscous stress tensor are

trXb- tr9X / 3yb 9v; \

tr"=^= -(t^' X? )

(27)

(28)

^= f^^ ?r- (29)

10

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GAE/ME/62-*l

(30)

■»■

^J + ^^ . (3D

and

^ " ^7- 3^) L9x 4 äV ^■

^ 1 n ^^ (32)

Equation of Notion. The components of the viscous

stress tensor are tabulated above. The remaining terms of

interest are

i^ ., 3K (33)

11

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GAE/MK/62-4

M

a£b(^) +^(^xl) , (36)

4(^)^^(f^) , (37)

and

_äiK

Cylindrical Coordinates

Continuity Equation.

(38)

(39)

% = ^33 = 1 (40)

^x = ^ ^ (41)

12

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GAi/Mj;/62-4

M * F ibfK) <? &(fü)*|i(f i/,)' ö (is)

Snergy Equation. The left side of equation (5)

becomes

tilthniK%*vMx)] * v.f>[^i(r+

^hhA^w.ws)]]. (43)

Also,

I*(V>^V61TS%V^") , (M)

(45)

and

13

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GAE/MS/62-i*

i. i. (ML- Z \ 1 i f ~ \

7 J6(^e) + a*(£^ . (46)

The comoonents of the stress tensor are

-re. £**_ ^£(4o*Tffl(v;)] , 7r

i^ . L ^h + 9?J , rrKt= tr1^- ^r

^=(rlr)[;I.H)4^

?i J + 2.T jp.

(^7)

(48)

(49)

(50)

(51)

and

14

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GAB/M2/62-4

^M'(Hr)[UH) + |^

li] ^-ü« (52)

Ration of Motion. In addition to the components of

the stress tensor tabulated above, the terms of interest

are

€W- -ill*U^) + i%(£««),

(57)

and

15

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GAS/MS/62-4

ifc V = -%+T§-rU")*iUV) c) / ^

li(1?H). (58)

Spherical Coordinates

x' ■ : V

XV^ 0

3» = K"''^!^ "9

r r'5>nx Q

Continuity Equati on.

X5-(() {59)

(60)

(61)

(62)

(63)

atf "" ^^^(^^J ^ r^relö(5/ne^l/e) +

1 2- I M\ (64)

16

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CAE/ME/62-4

Energy Equation. The left side of equation (5)

becomes

F Si* ö äf Lll ♦ I (K"*- *i>'+ V»")]i . (65)

Also,

\^S)J ^ rs^rfU^v.fr^^^J ,(66)

^V.f; : flVyF^YXtV.fFf] . (67)

and

|r sine aeU'«e £e) + ps^Tä^f U^ ) . (68)

17

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GAE/ME/62-4

The components of the viscous stress tensor are

7r -- tr0 = r »-ahlp-;+ r 9-aJ 3

£.*<* A.A**. ^F. -^/^^ -i 3^"

(69)

af J, (TO)

.•♦-^.- T[S^ä(^) ^•♦= i>»».

1- ilti ö a-ai . 5-f J, (71)

^- (?-|r)lf fhd'-Vj ^-77^lö(/6Tm«) +

^y. lTr^ , (72)

fr06- (^lT-)[>^(^K)v"^rfllö(\i^ö) +

i av. V- Si -6fj + Z^LT^.O], (73)

and

£<P<Pr

^ Jin 6 ^(p J + IV L H 3/rt Ö I «^ 4-

^ + V6 (LCA Ö )J f (74)

18

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GAE/ME/62-4

aquation of Motion. The terms of Interest, In addi-

tion to the components of the viscous stress tensor already

listed, are

rS/ne «99 yT > (75)

7e- at + ?ar(^W^7 ae +

rsmö aq) " "p. Co^ © i (76)

üL. iy<p ir sme dp , (77)

,JK

Tkf^)-7^.^) , (73)

19

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ü/h'/Mi'AJk-^

(r)r^)

i 3 rsmele(^0H+ firTeTfift**) "

V^Cöre * Z^6" , (79)

and

^K.

^ <?P •* sL

1 5 /^tofl\ i 5 r ae^ ■; ■" KSinö a^ (

F^ ■f- 2 COT ö ^(pe

(BO)

Parabolic Coordinates

x'-- A X = ^ X = (p (31)

CJn (B?)

^ 1.1. (S3)

$33 ^ ^H m'

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GAE/ME/62-4

9 ^ /6 (85)

Continuity Equation.

SnerSly Equation. The left side of equation (5)

becomes

(86)

'.f^JJ . (S7)

Also,

21

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.. .■.-.:.''**'|

ÜHC Mfi OJ-i(

v^"" *vt£Hj+^4ki^V?*H£wI . (88)

fV<^ = fll//^^^ +^Fj , (89)

and

J. a IJEL x] z d_ l, ^ ]

XT^ ^[/^(A+A ^1 * fXMdfifri) . (90)

The components of the viscous stress tensor are

llMd^i^)} , (91)

fÄM 54) J j (92)

22

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GA3/ME/62-4

V^w? V'PM rr*

(93)

A"^äA(^(A^ ^-^ 7^ a9J +vU^f^^^

tr^

CA+x) ̂ vi - ^fc)^ ^] , (95)

and

MTXtM^ VA +/7^7o l//^] (96)

23

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üAi/M.C/bJ-^

-; tatl".i _J H^tl' ii. i'tM- >; o(i!!'on<ii'a of ch • viacous

stress tensor are listed above. The remaining terms of

interest are

V„ JTH acp - ^(Afyu^'V^feT) > (97)

V "- at ^ ^ ä+^ aAC/J^^J + 2ji/^ 2M +

> (TO Jf ' VA (AtA4),/v - y<p iMÜ+M^ , (93)

V/,<9MW^)J f 7W 5<P , (99)

/p ^ = "^/ATS ä> •*" ßoS! äÄ (AiVAA) ■•■

/nfe) fr" >■ ^'^ f ^ , doc)

2t

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GAE/ME/62-4

I 3 i d

1 «P» . ?yZ,.1 ^^A (101)

and

J1K

/M1 5

(102)

Prolate Spheroidal Coordinates

x =A x\ M X = f (103)

* . a-

9' r CL x A -/K

(104)

»• , v

^-'^ (105)

25

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ü A ji/Mc;/6 ;.•-',

^33 Z Oi'W'lUl-M^ (106)

(107)

Continuity Equation.

QTCA^O^ <59 p^J ^ ö (108)

Energy Equation. The left side of equation (5)

becomes

y» 5 r i / .] 7 a/avJKT^) a^ Lh + I (\//+ ^% ^Jj (109)

Also,

26

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ane/tm/62-ii

7f jWij^f W'j'äüh*) IäUV«*--«"^^"*

and

TLIJJS:

(112)

The components of the viscous stress tensor are

fr^^MA = V[-X" 5A TT^ ^i +

(113)

27

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j \ :. 'A.: '■) - I

(114)

AMf _ N^CPAI rrMf= rr T

1 ^y •

(115)

ZACi-^^ ä.(A1-A1-)3/9^T V^ - OCAS?)^ 1^ J , (11 6)

+

(117;

28

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GAE/ME/62-4

and

^ (.f-Mi'^h + a WFfäd W . (n8)

Equation of Motion. In addition to the components of

the viscous stress tensor listed above, the terms of Inter-

est are

./ ^ A I V) a. fU^CAvT) 3 (ii9)

29

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Cr- . >!.•: ; '-h

(120)

dv( 1L— 1 > "- at + a/r^T1 ^ I/AM VV) ^-

ay, OVTA^-WL^ ^4 a<p j (121)

X ^ i [AM" £P 1 a r A -I ^ '% r "«-«A^aA -^o^vpiräA l(Al-i)?rA J +

Aräf^-^^f^ ^a'-^a^ (--22)

30

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,}.:./). „ ü2~4

M/l->kv ^A>

a-Zo^KTCT) ap(tr>,,J>)+ ofe?)'^ tr

M*

^ A (123)

and

,it<

£p ^7T hi.K ^ Mc/MV?^ Jcp ■f

5ET a

ZA «A fl.vo'-Da-^ Vtr^-f a/ov«^^ fr

avavM^-^) ^ H , (124)

31

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b. v l'u'JÖc-K

3i)hcTolcial Coordinates (Oblate Spheroids)

5. ? (125)

(126)

(127)

•»• \ I «- 9« r Ö- A> (128)

(129)

Continuity Equation,

3 at'

/PTT £/

nrz* d

(130)

Energy Equation. The left side of equation (5)

becomes

32

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(IAE/ME/62-4

dfe ^[ui(^Mi%v)]] • (131)

Also,

(132)

(133)

anu

33

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Lh ./W\'i\ '-h

(134)

The components of the stress tensor are

tTA^- h A <PA T-

1.

-1. 9^

(135)

(136)

(137)

34

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GAE/MS/62-i|

r /Äv:

r 2 3//ET., \ XA , i-Mv ..

0. (Al-^),/L ^J > (138)

FA £ //IZ5rl; \ ^A iZH, .,

2M A"- a n^a s^ vJ. (139)

and

35

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GA:-. t'U:, r.J-i\

£*' - iv- l^ioj^iiixf]^? VÄ) +

d^o)

Equation of Motion. The Important terms In the motion

equation are

n 3 ^ ^

M >

a AI-A

V^UAV<

I l^) +

KH iEg.. -Jl ^ CA^-v^ ^A^'-^

(141)

(142)

36

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GAE/ME/62-4

a^ vf^r^^UKp/+ Q.A>M 3^ 3 (143)

i rn^ 9 i s eLs/Ä^^^j^^r^^)

X>H

(144)

QMUW TT v + atA1--^1)^ fr ^ (145;

and

37

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GAVM.;'/6.M»

/TT^ 9 l d aMaSn*)^f^1^ tr^j f OXM 5^ (l?9f)

.^T^.A iklföffr"+&&$$'>*.

Parabolic Cylinder Coordinates

X -- A j .

e-

X ■■ M. ^ = 2

Continuity Equation.

dt 4 r+xi<9A(/A+>r |) v^)-<•

(146)

(147)

(148)

(149)

(150)

(15])

(152)

38

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ÜAE/MK/62-4

Energy Equation. The left side of equation (5)

becomes

(153)

Also,

^"hkk^+yJ'Wj"] 3 (154)

j)K/? = ^(1/,/-%^^ ^ v^fj 5 (155)

and

A £ . /ill ^ \ 2J11 (, . ^ \ 4-

(156)

39

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GAt./ME/62-i.

The comoonents of the stress tensor are

tr>M-trM>

Xi ^"-ti fA - [

^-^-rf./^l^.tJ, rifii. trw=(?-|T)lÄäÄf/Ä77rVA) +

(157)

(158)

(159)

^(w>|*W^&J- A+M ^M v.Mf^

AM, . z./xr w "I (160)

trMM- (yi-lrAh^äliü^rV,

UM U^^^l^hlM^ 2JK. \/ xA ,/ (At^ä/,-yA "" Stv^)^ VM 5 (161)

and

40

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;.r:^:i/62-4

^"= (v-lr)l]&i(rttvA)* UM d ^U(^W* l£]

(162)

Equation of Motion. The important terms in th(

motion equation arc

i = zi +1 yJ/.M 2* + zyM xt-dhiföxvÄ)4

A

I

f

^ o V Ül £// ,»/ \

i^Jfä 2M +h2i -

(163)

(164;

n ./ /IST iVx u 9/, 55,

41

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GAc./M£/62-4

(AfM)^frMM-h (ÄT7ö^h"AM , (166)

ifjratM^ VM +- (A+>M^1TMA 5 (167)

and

/fcV^-l^.^f^^lT«)

Xf I^te^^tl-Jrr"). (168)

Elliptic Cylinder Coordinates

x'-- A xz-- H x3-- e (169)

^i^ x^-t ~ (170)

42

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MiA'.-vfe-'*

^

a.^(^'■.M•)

<]

Xt

It

T

1

M'

«3 = CA^iKl-^)

(171)

(172)

(173)

Continuity Equation.

O-CA"1^ ^(^TF^^)^-Ji(fl/2) = 0 (174)

Energy Equation. The left side of equation (5)

becomes

Vj")] ^ %h[uAW^vs+vsi\, {175)

Also,

43

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0AE/M£/62-ii

jVißi - j>lvJ^VMi *-Y,ß,], (176)

and

4 ^(7p? ^) = ^5il(^v p + -kal 2.

The components of the stress tensor are

(173)

(179)

(iSo)

(131)

44

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GAE/ME/62-4

(192)

5-5E 3 /. ...v 3v,i r2 3 //75pvy \

a (A1-/,»)^ V; + atTFif-M^ yHi 9 (i83)

and

^^ £ fa—n i/) ^^1 n W* a(A1-^ a/HvA ■^v Üit J2 J +■ ^T^t . (134)

Equation of Motion. In addition.to the components of

the stress tensor listed above, the Important terms In the

equation of motion are

45

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GAE/ME/62-4

f.=

(135)

/.^.^(^ , (166)

VAI OST ^* v/ ^v* (137)

öSS^^^Ä^-^^, (133)

öTS^V. f-^5^1;.^ (159)

i[6

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GAE/ME/62-4

and

(190)

Slllpsoidal Coordinates

X'a A Xlr >H x3-- ^ (191)

(192)

(193)

(194)

9= M (a,x-A)(bt-A)(Cl-A)r^->HKbl-^)(>M.<;x)(a.i-y}ai-y)(ci-v)( 195)

Continuity Equation,

47

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I

GA.-/H.-/D2-4

^/^-yXb^-vXc^v) P (^y-A)(y-/4)\p|/ü) = v~X)(y-M\ 5vl/^-A)(y-/4) qyj) = o (196)

Energy Equation. The left side of equation (5)

becomes

firth A{\\vH\y:)] +

I (197)

AlSQj

43

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GA£/Mi/62-4

l/.^fV^^J, >l

f l/^ = ffvAFAf V^PI ^ ^fj,

(198)

(199)

and

(w-A)(y-^) 9MU^-^-A5 ÄX) +

lU^-nLtf-tXQ-y} H. U-^U-M) ä)>U(>>'»U-M) (UMU-M) £»] . (200)

The components of the stress tensor are

V^- h-M - ^r hi (0L^*)(b*-Wcl-x) 9 /_! ^-A

l((il-*Xbl--MHH^:) £ /I , a (201)

49

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GA-'Vi'iVoi-'l

^«y ^v. f W-MW.^(M^>^ II y \ Ir = TT ^ rU/ M-^ a^lTÄTM ivy

(202)

(203)

AA tr- - (^- ir-)

"e/Cat-A)at-Ayc:t-A) 9 i v

Z ^a.1-y)(b>->0(<:t->» 9_ {H^)i)>-M) ^ )] U-W-H) dy>[Uy-*)U-M) ^jj +

V. +

y/(CL,--^)(bl-A)Ccl-A)(M-AUy-Ab V A

JL / i(ll-M)(^-^)(c%-M) yK.-Ä i iÄ-M)(i>-M) V^

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GAS/te/62-4

2/^-M)(^>u)(>u-g^ j / , \ u-^Hy-^) ^MinM-ÄüPvM) yM J +

and

2 /((L^AKb^-AMc^AT .

A->K V (A-VXM-V) Vy J i (205)

51

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GA2/M2/62-4

Z/^-^g^M^vu-c^ 9. (y-M)(M-^ d*[i (M-AW-M) (UM-W-M) KA)

/A-y

OA)^ (V-ZM)^ "y +

/(a'-yXb^yj^-vj^-^^-yj ^J . (206)

Equation of Motion. The important terms, in addition

to the components of the stress tensor listed above, are

5?

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GAE/M2/62-4

(207)

r 3^ lit RgSSEME?-^ //—• \/\ tM

= at ■♦• A-MJ FA aAl/Ai-A VJ

I y» [{äEIWJE?EEF> £ I rr— \/ \

^1 H^KäSSSS^ v/ /CT^JS^ (208)

/H -/ ^(/T^Vy) ^

c^y

y-A (209)

53

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GA£/K£/62-4

-3- K. kay-Mr-Mc^) d? rap fli.K ^ '^J (M-X)(y-A) ax "+

2.

— ^i -__ z»>({?-Mlr ) +

(a^(b^AU (gMMc^A)^ (b^AVc^) .AAA

AM-AVy-AKa.1-AXbl'Ayc,-A^ rr

(210)

54

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GAS/ME/c2-4

vi*

/^ hi.l ^M

o^b^Wa^^uKd^^^ ->• (b^(<:v.>u) /j\MM

T4 -A)(^-MXflLl->M)(bv-^ (>H-C^

(211)

and

55

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GAE/HE/62-4

*») »p a> ^"

yU

JL

~J yrj aAl/^rtryA)

/CA-y)^-^ av (/^MÖa^JcMO fr ^j -

(6.t-y)(b1-y)^ (^-^xC'-y) -^ a1-»^1-» ^ /(ax-y)Cbl-y)(c,'-y)(A-y)(M-y) tr yy

/7FA(V-AV/V M* t- /7rT(V'>M)l/v/r . (212)

Confocal Parabolic Coordinates

X1-- A X1- A X* = )> (213)

(214)

(215)

56

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GAE/MS/62-4

^33 = ^ra.-V)(b-vi (216)

rA-M)v(M-y)VA->0 g ? ^^rÄ-^b-AVM-Ä.)(6-^){d-y^6-y) (217)

Continuity Equation.

u-sHM-y) d)>{iU~y)(M')» fVyj* 0 (218)

Energy Equation. The left side of equation (5)

becomes

i (v;+ Ct i/;)Jl. (219)

Also,

57

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ÜA3/ME/62-t

\/M^ f Vvfr^)]^ l-M^I-Ä*tmvivj^

j)Vif^ f[v,F, ^^F^^ VyFy] ,

(220)

(221)

and

The components of the stress tensor are

^■rr^-rUm^hiT&y.)

(222)

(223)

58

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GAE/ME/62-4

IT --fr ' TTilV x-M dÄTT? y)

(224)

MV VI^M rrMy=VyM- T

(225)

CA-yvx-y) ^y UCA-y)(>M-yy Vv )J +

T n 3A 1/(A-MXA-^ VA + (A-^i^^A-v)^ VA

^a-Ayb-AVA-xXA-y) VA - yM y (ZTÄK^) VM -

A-V J Vy] 3 (226)

59

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GAE/ME/62-4

h-MM = (^ i JlMMM 9 fh ; \/\

2^M-d.)(b^V 9 I. . w \ i

i!M-y)(A-y) aymA-y)CM-y) /„/ +•

^(^M-a-6) v.- 'M

M-^ vry-AKV-^ ^ (227)

and

60

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GAE/M3/62-i|

ZJJM'XHl'Ml £ / r- w \ fM-vTU-M) aM (/a^ )f>u-y) //4) +

^L 1 //5Z2ZEF \/ U -^ /SZSET w

(228)

Equation of Motion. The terms of Interest In the

equation of motion are

■+■

2^ A-y

f(A-yKfe-y) £ / . . w \ i" M-» aylvÄ-y VA) +

-A / (A-. AVö-A^ M)(A-)» (229)

61

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GA£/ME/62-4

zvy MlgSS i. irr? \i \ +

_y!Lv /ESESr v/ fSSEg , ^.

rt ü^TM'V) + >M v?^Atery) , (230)

iy •- at- + y-A y A-^ SAVM-^ V>

IKM /(M-<0(b->MV i- /.—r W ) .

p^v \W->W-MS > (231)

62

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GAß/MS/62-4

9\ 0 /(a-A)^-^' £P

/CwöcTT)

i /(u-a.Mb-M) £. /. T^AM)

Q. + b - ZA Va-dL)(A-b) ^

2- , KcL-yXb-y) £. AV^ 7r (232)

63

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GAS/W62-4

'(A-MKM-y) a^ iüM-<i)(t>-M) fr^) ^

(A

a_f t> - 2.M. if-»".

and

f (233)

64

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GAE/M2/62-4

M

ii»-X)i)>-M) 5y(/(d-y)(b-y3' ^ ; +

M-g^ ^.AA JEMS t?"- (A

(A-y)?"-(M-^^ n" 4-

ÖL+- fc ^ 2 y

V^-y)fb-vKy-AVv-^ri /^ yy

_!_ l(a-AMb-A) £ vx

?r ^ (234)

Conical Coordinates

r- A x1-^ x3= ^ (235:

8- - ^ (236)

65

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GAE/ME/62-4

qix- (M^b4)^*-^1) (237)

q^ - (bx-^x)fc»-y») (238)

q~ (Mx-bMCcl->uM(bl-y»)(cl-y») (239)

Continuity Equation.

i/IE22E35 iL /,—^ ,/\ A ^-y- ^V l/^M^ f Vy ) = 0 (24o)

Energy Equation. The left side of equation (5)

becomes

66

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GASAB/62-4

(2^1)

Also,

4^(fe K^ij)' il-J^(v^^^A +

^Vif. = f [ V, F, f V;P^ + K,FJ , (343)

and

67

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GAE/ME/62-4

^(/MT^T|!M)

+

i /ä^y^Cc^yO ^ A /M^-y1- Z)>(jMx-y1'' i^) , (244)

The components of the stress tensor are

/ if A«1-^»- a^ J j

A If /Ax-y* 9y J j

(245)

(246)

A

tr ̂ .1Y^- Y[iu^-6l)^.^)|M(^7lV,) +

7 ^-yO^-yO ^y (CT^ VM)] 3 (24?)

68

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Gb?.A<\z/62-h

^oz-wIM^K UM*'WC*-M*) 3

MA« tr^-(>e

S A

A VA

2M

r/4

bx 4 C1 - Z

(249)

and

69

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GAE/ME/62-4

lYy,,-(^|T)[j'JA(^Vj

{TM£V5U^ä& a

®

111 b1 4 c^- ~ z ^ ^1. (250)

Equation of Motion. The terms of interest in the

equation of motion arc

^ = at ■*■ VA äÄ + X / x^-y- a^ 4-

A y /u-i'-y- a^ A 7 ^ (251)

70

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OAE/toE/62-4

f„- » ■ Hi/,.., K A 5\ s\^vJ

^

(252)

,J!(

^ ^li,,

i^- ^^ £

(253)

(254)

71

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GAS/ME/62-4

(255) I y

V/Cb^-V^CC'-y^ /v /Cb--v^^-y^ . ^——^

A(/Ml-VOJ/C ^ (256)

72

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C/^/Mi/6,-J|

IV. Conclusions

A report of this nature has no conclusions In the

usual sense of the word. The methods used In arriving

at the final results were not new. It was known at the

outset that they would produce valid results if they wore

applied correctly. This project was undertaken because

the equations of fluid mechanics are not readily avail-

able except in terms of three or four of the more commonVy

used coordinate systems. The tabulated equations in Sec-

tion III arc, therefore, real1:/ the "conclusions" of this

thesis.

73

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GM/m/62-H

Bibliography

1. McConnell, A.J. Applications of Tensor Analysis. New York: Dover rubUcatlons,~Inc ., 1957.

2. Morse, P. M., and H. Peshbach. Methods of Theoretical Physics (Vols. I & II). New Yorkl McUraw-Hlll Book Co., Inc., 1953.

3. Page, C. H. Physical Mathematics. Princeton, N. J.: D. Van Hostrand Co., Inc., 1955.

4. Sokolnlkoff, I. S, Tensor Analysis. New York: John Wiley & Sons, Inc., 1951.

74

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GAS/Mi/62-4

Appendix A

Description of Coordinate Systems

75

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GAii/Mi/öS-il

The coordinate transformations presented here werr'

taken, with minor changes, from the work of Chester H. Pare

(Rcf 3: 96-107).

(1) Cartesian cooräinates

x»x -OÖÄXtOO

y o y -00 i y Ä 00

z = z -oo < z - oo

g., s S»v« GM« -

and the surfaces x. y, or z s constant are planes.

(2) Cylindrical po"!ar coord Ljiates

x - r cos ©

y - r sin 0

z = z

with the variable ranees

-oo < z s oo

0 i r £ oo

0 * 6 * o fr.

The surfaces are:

z =• con^' sv planes

r = cc.nz''. ^ cyHndors

Ö = const ^^ ^1 rncü ' hrour'" V:::-. z-v.:■:'.■.

Wc have:

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GAE/ME/62-4

Flg. 1

Confocal Parabolas

with a Common Axis

77

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GAE/KJ3/62-4

(3) Spherical polar coordinates

x = r ein ecos <p

y - r sind sln^

z * r cos &

0 s r ^ oo , r r const ~ spheres

0 5 V s 2V, cf = const ~ azlmuthal planes

0 ? 9 - 7r, ö = const /v circular cones

9"--1 > 9vv= ^i 3ii» ^J'^vö

(4) Parabolic coordinates

Two sets of coordinate surfaces are generated by

rotating the parabolas of Pig. 1 about the x axis which

Is then renamed the z axis. The third set of coordinate

surfaces are azlrauthal planes through the newly relabeled

z axis.

The transformations are:

x - /AJA cos (/>

y = /XM sin (p

z - ^

0 < A£ooj A = const/v paraboloids:

x1'+ y + 2Az = Av

0 ■£ y4 < oo j /> = const /^ paraboloids:

xN y - 2^2 = z^1-

Oi<p"£Z)T; (}?= const ^^azimuthal planes

3"- 4A , 3"' ^^ , 5" r ^^

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Y

rig.

Confocai illipsos and Hyperbolas

(5) Prolate spheroidal coordinates

This coordinate system is constructed by rotating the

curves of Fig. 2 about the x axis which is then renamed

the z axis. The coordinate surfaces which are generated

are prolate spheroids and hyperboloids of two sheets. The

third set of coordinate surfaces are azimuthal planes

through the newly renamed z axis.

If we let A H cosh oc , /^= cos ß , we have

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x - a/ Av- 1W 1 - MV cos (J>

y = a/Av- 1 /l ->AV sin 9

z r EXM

iiA^öo, A» const/^ prolate spheroids:

*^v + Z.v - /^ vM + Av - CL

-1-A{* 1 j /^ i const/^ hyperlolds of two sheets:

O < (p< 2.tr, (J) -s const ^ azlmuthal planes

(6) Spheroidal coordinates (oblate spheroids)

This coordinate system Is constructed by rotating the

curves of Pig. 2 about the y axis which Is then renamed

the z axis. The generated coordinate surfaces are oblate

spheroids and hyperbololds of one sheet. The third set

of coordinate surfaces are azlmuthal planes through the

new z axis.

x zaA^ cos <p or r = a cosh^cosß

y = a A *A sin cp z - a sinhet'sin^

z = a /CÄMUTV) A = const /-o- oblate spheroids:

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M, ~ consi /v/ hyperbololds of one sheet:

(P ■= const/v» azimuthal planes

wiih the variable ranges

' 00 < o<* & 15 A -£" a> ,

We have

>v ^r^\ 333= a'A^1

(7) Parabolic cylinder coordinates

The traces of the coordinate surfaces of this coordi-

nate system on the xy plane are shown In Fig, 1.

y r /AM

z - z

0^ A? oo . A - const /u parabolic cylinders, u7,+ i^X - A

Os^-Cö M- const^ parabolic cylinders, tj*- 'J-/MX»/^('1

-Oo<2Seöi ? " conöl^u planes

A + M XiM

(8) Elliptic cylinder coordinates

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The traces of the coordinate surfaces of this coordi-

nate system on the xy plane are shown in Fig. 2.

or x s a slnlWsin fl

y 3 a cosh Ycos fl

x c a /A%-J /l-xT'

y =• a A H

z r z z = z

A ~ const ^v elliptic cylinders, ^»Tj ■*" A1, * ^

At » const,-Vi hyperbolic cylinders, ^ - j^Tt m d.'

7 a const/u planes

with the variable ranges

- 00 £ ey* + 00 .

Ö £/9« tr ,

1 ^ A ^ «D.

-00* %< 00 ,

We have

(9) Ellipsoidal coordinates

* ■' feLv-bv)(a^-Cv) (Jin/

2 ^ (a.l-OCb,l-c^

-to<xf c><>{< l)Vv<a.

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The surfaces are:

A - const n ellipsoid:

M - const:/v hypcrboloia of one sheet:

xv bv «*

ä^T, + t7"^ + I^M --l > c*- * M< ^^

y = const /^ hypcrboloid of two sheets:

Xv ^ ■?LX

Also,

i ^-AMV-A^

5„ ' -9 Ul-XVbl-AUcl-A)

5 l\

and

(lO) Confoca1 parabolic coordinates

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The transformations are:

^ * b^Z

* a - b

The surfaces ^, ^, and ^constant are the paraboloids

A "*■ A(A-öL) + A(A-b) ::: i

— bx ?l

with

00 ^ >)< <L< M< h< X < OO

Also

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and

1 U-^^-u)

(11) Conlcnl coordinates

The surfaces ^, >M , and V constant arc the spheres

x + y + z = A and the two cones

^v ^/tv-^ ^/F^C1 = 0 and

yl ^ y^-b1 v yl- c1- = 0 i

where 0-sy<b*^«:C j O^A^Ä?.

The coneSj JL\S constant, Intersect the planes, z « constant,

In ellipses. The cones, y= constant, intersect these z

planes in hyperbolas, but Intersect the planes, x « cons-

tant, In ellipses. Hence, we can visualize the cones as

being elliptical cones centered about the z and x axes.

The transformations are

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H - i>Vb*.c*) j and

? = Cx(cl-SM .

Also,

and

9" ' I >

^33= C6l-yvKci-y^ .

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C

Appendix 3

Derivation of Basic Equations

of Fluid Mechanics

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The derivations shown here can be found, In slightly

varying form, in the works of Sokolnikoff (Ref 4: 290-324)

and McConnell (Ref 1: 270-282), among others. These

specific forms were, however, firsu shown to the author

by Lt. Ray M. Bowen of the Mechanical Sngineering Depart-

ment of the Institute of Technology.

Equation of"Continuity

The equation of continuity can be expressed in inte-

gral form as follows:

fthd) f ^'W^t" = 0 . (B.l) d Si

Application of Leibnitz's Rule yields

(B.2)

By the Divergence Theorem

Ll(^ JK(,)(fi^l■))id^ | s 0. (B.3)

Then, since volume is arbitrary,

d al + (f^4*).,- = o, (B.4)

but 88

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ijV% = Jfzk'iljft1) . (B.5)

(Ref 1: 155). The continuity equation then becomes

a/ + q aitifi' fv1) r 0 . (B.6)

The physical componcn"s of the contravarlant quantity f

arc represented by ^tim]^< If we denote the physical com-

poncnts by ehe symbol v^ , then cr •/| . ,.- We can then write

the continuity equation in its final form:

at + ^ ax11/37^ fVO = 0.

Energy liquation

The energy equation can be written in integral form

as follows:

Application of Leibnitz's Rule yields

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iL)^"'^ o(J t («, ü-,' f F 'af> - 44V afs, (B.9)

and, by the Divergence Theorem,

Then, since the volume Is arbitrary,

(^V'M.it jKf1- f.c . (B.11)

By expanding and subtracting out the continuity equation

we obtain

^ [ ft (wt i uju V V'(ut x ir^O.-J-

UcY^Xt ^^r'-f.c . (B.12)

But

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U ~ h - J (B.13)

Substitution of (B.13) into (B.12) yields

where v/e have also made use of the relationship

After simplifying and rearranging, the energy equation

becomes

5? + (^IT^)^ + ^if'" f.L . (B.16) )

or, in terms of physical components

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flhih*i YiVi) + J$$§k'(h+iKK)]* It ■*■

/? & (fe ^ )riJ) ^ f K' r, - ^ Cfc^B., 7)

aquation of Motion

The oquation of motion can be written in integral

form as follows:

3iLn'idy--Lr\ds->Smff'citl (B.)8)

where

>'j = • p^ + Tr1' . (B.15)

By Leibnitz 's Rule

/y(t) ät (ft/4) df +i^f t/^\ (O'^-

(B..19;

and^ by the Divergence Theorem,

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LJIiif^) *(f ^J)Jdf ■J[((ä{Vij VF'k(B.2o)

Then, since the volume is arbitrary,

^(fir'M/^V),^ Vü;. ♦ j'f4', (B.21)

Now, after expanding and subtracting out the continuity

equation, we have

l(¥^<y)-r%+fF\ (B.22)

or

r-i>r'= Ki,, ft -f i 5 (B.23)

wher

i - 31/^ f.H f 1/

Scrt

- at -^ ^ ^ cr = rt (B.24)

Equation (B.23) can bo expressed in covarlant form a;

^n^K-- f(^-Fa (B.25:

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Appendix C

The Three Basic Equations

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Continuity aquation

t/+4M7!£? fVi]-o (3)

Energy Equation

(5)

Equation of Motion

s /^T7o ^j.K ' f Cfc -f/) (12)

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GAE/W62-4

Vita

Bradley Sutter was born

the son of

He graduated from

In In 1948, and spent one year at the

University of Minnesota before entering the United States

Naval Academy In June, 1949. He was graduated from the

Academy with the degree of Bachelor of Science in June,

1953. Since completing pilot training in August, 1954,

he has served as a flight instructor in the Air Training

Command and as a pilot in the Strategic Air Command, He

entered the Institute of Technology in February, ^ö1 .

Permanent Address:

This thesis was typed by Bradley Sutter,

96