52
EIR-Bencht Nr 346 Eidg. Institut fur Reaktorforschung Wurenlingen Schweiz Rapid Depressurization of a Compressible Fluid: a comparison between usual 1 -D numerical analyses and a 2-D experiment based on the shallow water analogy M. Dang, J. F. Dupont, H. Weber i? Wurenlingen, August 1978

Rapid Depressurization of a Compressible Fluid:

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EIR-Bencht Nr 346

Eidg. Institut fur Reaktorforschung Wurenlingen

Schweiz

Rapid Depressurization of a Compressible Fluid: a comparison between usual 1 -D numerical analyses and a 2-D

experiment based on the shallow water analogy

M. Dang, J. F. Dupont, H. Weber

i? Wurenlingen, August 1978

EIR-Bericht Nr. 346

RAPID DEPRESSURIZATION OF A COMPRESSIBLE FLUID:

a comparison between usual 1-D numerical ana­

lyses and a 2-D experiment based on the shallow

water analogy

M. Dang, J.F. Dupont, Dr. H. Weber

Wtirenlingen, August 1978

This report refers for work performed within the cooperation of

BBC Aktiengesellschaft Brown Boveri ft Cie, Baden

Brown Boveri ft Cie AG, Mannheim

Eidg. Institut für Reaktorforschung, Würenlingen

Gebrüder Sulzer AG, Winterthur

Hcchtemperatur-Reaktorbau GmbH, Köln

Kernforschungsanlage Jülich GmbH, Jülich

Nuclear-Chemie und Metallurgie GmbH, Wolfgang

Schweizerische Alurti'jiiiin AG, Zc.ich

on the development programme for nuclear power stations

with high temperature reactor and heliumturbine (HHT), which

is sponsored by the Federal Republic of Germany, the state

Nordrhein-Westfalen, and the Swiss Government.

Abstract

The rapid depressurization of a plenum is a situation fre­

quently encountered in the dynamical analysis of nuclear gas

cycles of the HHT type.

Various methods of numerical analyses for a 1-dimensional flow

model are examined:

- finite difference method

- control volume method

- method of characteristics

Based on the shallow water analogy to compressible flow, the

numerical results are compared with those from a water table

set up to simulate a standard problem.

CONTENTS

Notation Page

Introduction 1

A. Basic Equations of conpressible fluid flow 6

A.l Conservation laws 6

A.2 Intrinsic constitutive equations 6

A. 3 Extrinsic constitutive equations 7

B. Numerical Methods of Analysis 8

B.l Finite Difference Method (PDM) 8

B.l.l local conservation equations 8

B.1.2 local one-dimensional equations 8

B.l.3 Explicit time derivative equations 9

for p, p and m

B.l,4 Space discretization 10

B.2 Control Volume Method (CVM) 12

B.2.1 Space subdivision into control volumes 12

B.2.2 Conservation equations for con- 13

trol volumes

B.2.3 Standard simplified form of the CVM 13

equations

B.2.4 Remarks 15

B.3 Method of Characteristics (CHM) 16

C. Experimental investigation based on the shallow 18

water analogy to compressible fluid flow

Page

D. Application to a Standard Problem 20

D.l The Standard Problem 20

D.2 Results 21

D.2.1 Shallow Water Analogy 21

D.2.2 Finite Difference Method 24

D.2.3 Control Volume Method 26

D.2.4 Method of Characteristics 26

D.3 Comparison 27

D.3.1 Comparison of the numerical methods 27

FDM, CVM, CHM

D.3.2 Comparison of the 1-D Compressible 27

Flow Model with the 2-D Shallow

Water Flow

D.3.3 Influence of the number of discre- 28

tization zones

E. Conclusions 29

Appendix 31

References 34

Notation

Symbol Description Units

c veloT*. vy of sound £ m/s ]

C- Characteristics

CHN Method of Characteristics

C specific heat at constant pressure [ J/kg/K 3

C specific heat at constant volume £ J/kg/K 2

CVH control Volume Method

D. hydraulic diameter of flow C m 1

FDM I finite difference method with dis­

continuous treatment of the area

change

FDM II finite difference method with con-

tinous treatment of the area change

h depth of water [ m ]

HP high Pressure

i enthalpy per unit mass [_ J/kg ~]

v2 r i - i + -r "dynamic" enthalpy per unit mass L J/*9 J

Cw/n2 1

r N/m2 1

C N/m2 j

r w ;i L W/m3 j

j

LP

m

Nu

P V 2

P0=P+(K"1,2

Pr •

Q •

q

heat flux

low Pressure

mass flow

Nusselt number

pressure

Prandtl number

total heat current

heat current density

Symbol Description Units

R Gas constant

Re Reynold number

£ area of cross-section £ • 3

SHU Shallow water

t time L * l T absolute temperature Q if]

u internal energy per unit Mass £J/kg 3

v fluid velocity f a/s ]

Cr

heat transfer coefficient [ w/m /K ]

'P K = — adiabatic exponent

cv

A thermal conductivity £ W/M/K ]

p density [_ Xg/m J

5 friction coefficient

T friction tensor CN/,n J

- 1 -

Introduction

The analysis of rapid pressure transients within a gas tur­

bine circuit has become a major safety concern for gas cooled

nuclear power plants using a gas turbine in a direct conver­

sion cycle (HHT project in Europe ref /5/ and GT-HTGR project

in U.S. ref /6/ and /7/). The reason for this is that hypo­

thetical accidents such as the total deblading of turboma-

chines Must be taken into account as design basis accidents

(Fig.l). Such accidents induce a very fast pressure equali­

sation between the high (70 bar) and low (24 bar) part of

the gas turbine cycle (Fig.2).

Various computer codes have been developed which solve the

1-D flow dynamics equations with numerical schemes based

either on "finite difference" (ref /8/, /9/) or on "control

volume"(ref /10/, /ll/) techniques. The main problem is to

simulate the dynamical behaviour of the whole plant without

excessive computing time. The code PLAYGAS developed at EIR

was found to be a good compromise to meet the above contra­

dictory requirements.

To assess the validity of computer models several available

dynamical measurements from fossile fired power plants with

closed air turbine cycles have been checked against numerical

results. The examined transients varied from "load following"

and "loss of load" operations (ref /ll/) up to an emergency

shut-down" with rapid air relief over exhaust valves (ref /10/).

For this last case mass flow inversions and depressurization

rates of up to 50 bar/s could be satisfactorily simulated. In

this way validity of the usual numerical models can be con­

sidered as demonstrated for the above category of transients.

However, the accidents postulated for luclear gas turbine

cycles involve much higher depressurization rates in the high

pressure part of the circuit, about 200 bar/s in the large core

- 2 -

inlet or outlet plenum and even up to 2000 bar/s in some ducts

(Fig 2). The question now arises of the validity of the usual

numerical models for these extreme transients, i.e. the vali­

dity of

• one-dimensional models

• "control volume" versus "finite difference"

methods

• large space discretization

• neglecting pressure discontinuities (shock

waves)

With this report it is intended to answer some of the fore­

going questions by presenting:

• an overview of the usual 1-D numerical treat­

ments of the gas flow dynamics

• a comparison between 1-D numerical computa­

tional results and 2-D measurements obtained

with a shallow water analogy experiment for

the case of the rapid depressurization of a

large volume through a long pipe (standard

problem)

The "shock wave" has not been examined here since the stan­

dard problem involves only depressuri*..tion transients and a

rarefaction wave can never lead to a shock wave. Consequent­

ly some conclusions drawn here apply only to the high pres­

sure part of the circuit. The main conclusions are the fol­

lowing :

• no basic physical difference exists between

"control volume" and "finite difference"

methods. They even produce identical results

when the numerical schemes described here

are used and provided that the same space

- 3 -

zoning is applied to both Methods.

the number of discretisation zones can

be varied in a large range for the stan­

dard problem without significantly affec­

ting the results.

The 1-D numerical treatment is in a good

agreement with the 2-D experiment, par­

ticularly for the pressure behaviour

within a large v*. li

Usual 1-0 flow dynamics computer models, such as PIAYGAS, can

be considered as a reliable tool for the analysis of very ra­

pid transients within closed gas turbine cycles, at least for

the high pressure part of the circuit. The validity of these

models for the low pressure part of the circuit, when shock

waves are involved, should be further examined.

Zntnreoolar

Thexiwl Sh ie ld

E l«c . H»-Turbln« HP Oaqpcwaaor LF O a v m n r

FIG. l SCWMKTIC VIEW OF THE HELIUM FLOW PATH IN THE HOT OCNOVB PRESSURE VESSEL.

HYPOTHETICAL ACCIDENTS J TURBCMACHINERY LOSS OF BLADES OR MAfSXV. FAILURE

OF A PBCUPERATOR SUPPORT PLATE.

- 5 -

BO

70

60 -

50 -

40 -

30 -

20 0.2 0.4 0.6

Time (s) 0.8

2 -

± I 0.2

LP-Recuperator Turbine

Reactor Precooler

i.

HP-Recuperator LP-Compressor

— Intercooler HP-Compressor

J I 1 I I 0.6

Fig. 2

0.4 Time (s)

DEBLAD1WG OF THE HELIUM TURBINE: TIME

BEHAVIOUR OF SOME PRESSURES AND MASS

FLOW RATES.

0.8

- 6

A. Basic Equations of Compressible Fluid Flow

A.l. Conservation Laws:

The unsteady motion of a three dimensional compressible fluid

is governed by three conservation laws: mass - energy - and

momentum-Conservation. The integral form of the three con­

servation equations applied to a fixed volume V with boundary

3V can be written as:

lp/7/pdV = - //pv»do A-l

V 3V

§£///(pu+p|-)dV = -//p(i+|-)v-do+Q A-2

V 3V

|t///pvdV = -//pv(v«da)-//pdo+//T«da

V 3V 3V 3V A-3

This system of equations is completed by the following two

types of supplementary equations:

A.2 Intrinsic Constitutive Equations:

The thermal and caloric equations of state for an ideal fluid

with constant specific heat are:

p - pRT A-4

u = CvT A-5

and the following thermodynamic relationships apply:

1 - u + £ - c_T A-6 P P

- 7 -

C = C + R A-7 P v

£ - « A-8 V

where n. is the gas constant of the fluid, C and C the speci­

fic heats and * the adiabatic exponent.

A.3 Extrinsic Constitutive Equations;

For three-dimensional flow, the total heat current is given by

the well known Fourier's law:

Q - / / 8 V J • da = - // 3 VA |S dok k = 1, 2, 3

k

\ denoting the thermal conductivity of the fluid. This ex­

pression is, however, nnsuitablr for one-dimensional treatments

and must be replaced by the empirical equation:

Q » // aAT | da | A-9

with a = 2H-2. , Nu = Nu (Re, Pr)

where a denotes the empirical heat transfer coefficient, and

D. the hydraulic diameter of flow.

On the other hand, the friction-tensor T for a Newtonian fluid

is given by:

dv. ?V. 3v, T i k - a < ^ + j ^ + b irt ' 6ik

- 8 -

for three-dimensional flow:

For one dimensional flows, friction is considered by the addition

of a pressure drop term of the form

«Pfr (x) = n *te& ax A-IO

to the pressure.

B. Numerical Methods of Analysis

B.l Finite Difference Method (FDM)

B.l.l Local Conservation Equations

A local form of the basic equations is obtained by applying the

theorem of Stokes to the surface integrals:

3p ,. -*• B-l ^ = - div pv

+2 *2 |^ (P (u + |-)) = - div (pv (i + |-)) - div 3 B-2

9 - (pv) - - div • (v p v) - grad p + div T B-3

B.l.2 Local one-('imensional equations

In a one dimensional coordinate system with voliw> element

dv = S (x) dx, the expressions for div and grad are:

div - > sTxT k (s(*> >

*rad ~> k.

- 9 -

Equations B-l to B-3 then become

H - - sW h «"s ««> ' "-*

It (»(» + 5-)) --ST50 fc «»vS(i4|-) ) + 6 B-5

I t « » » » - - s W S i l o v S - v ) - I f - f ^ ° i v i v - B-6

For the heat-flow term -divj, the 1-dimensional expression

A-9 in the local form with the thermal power per unit volume

u S(x) 3x

must be used. For the frictional forces the expression A-lO has

been inserted.

B.1.3 Explicit *--tne derivatives equations for time derivatives

p, po an m:

2 If the variables p, m = pvS(x) and p = p + (x-1) %r- are

O 2.

chosen as differential variables, the partial equations B-4 to

B-6 can be written as:

i£ - I 12! n 7 at " S 3x

^ - - ^ lx-'" < i +T" * «-»« B-8

If - - k «->-s If - 2Jri»i- "-'

- 10 -

The corresponding transformation of the equations, together

with the algebraic expressions for i, v and p are s.»own in

the Appendix.

B.1.4 Space Discretization

The finite difference method consists to replace the derivatives

in the local conservation equations by finite differences.

The space under consideration is first divided into discrete

zones and the physical variables are then determined at each

node. For one-dimensional flows in channels, axial zones of

length Ax are considered as shown below in fig. 3.

k-1 k+1 Zone k

Fig. 3 Space Discretization (FDM)

- 11 -

The equations B-7 and B-8 are now applied at the zone centres

to determine the dynamic pressures p . and densities p. by

substitution of the gradient terms on the right hand side of

the equations by finite differences of the corresponding values

at the zone boundaries:

pk I k k-1 _ * . _ i * *_± B-10 dt SR Ax

dP„ L. it.n ("v^ v_mt_i *„ i,_i > o,k _ _ (*-l) '"Vo,k "k-1 o,k-l' ,K ,. • ,,

~aT sk AX + ( 1 , qk B n

Similarly, the equation B.9 is applied at the zones boundaries

to determine the mass flows m. by substitution of the gradient

terms by the finite differences of the corresponding values at

the zone centers:

!mk (Pk+ i s k + i " pk Sk ) ( mk+ i v k + r m k V dt AX AX

B-12

A - Sk+l~Sk , C v - * i

+ Pk —Ax (2D^ 'mkfVk

It should be emphasized that the discretization scheme adopted

in deriving equations B-10, B-11 and B-12 was chosen in preference

to many other possibilities according to the following physical

requirements:

a pressure or momentum disturbance is propagated

either to the right or to the left of the flow direction,

a thermal disturbance is, however, only propagated

downstream.

- 12 -

A detailed derivation of the finite differences equations B-10,

B-ll and B-12 is given in the Appendix.

B.2 Control Volume Method (CVM)

B.2.1 Space Subdivision into Control Volumes

The flow channel is divided into 2 types of control volumes as

shown below in fig. 4.

Control volumes with

mass and energy con­

servation

Control volumes with

momentum conservation

Fig. 4 Space Discretization (CVM)

- 13 -

B.2.2 Conservation Equations for Control Volumes

The integral equations of conservation A-l, A-2, A-3 applied to

the 2 types of control volumes considered in fig. 2 give:

ft "'k pdv " " (ik " "k-l>

. 2 dt ;//k P(»*T)«V = -(Vo,k-Viio,k-i) + ̂ k

^ ///pvdv = -(Pk+1sk+1-pksk) + pk (sk+1- sk)

I • I ~

- (mk+i vk+i • rak V - ^ f e r W ^ k n

where the indexed variables of the right hand sides are local

variables at the boundaries of the control volumes.

The following approximations are now introduced:

fffk pdV = Pk Sk Ax

v2 1 v2

/;/pk(u+^-)dv = ;— /;/kp dv + ///k P|- dv

, 2

" Z=I pk sk Ax + / ; / R P T dv

= r p . S, AX >c-l *o,k k

///k pvdV = mk Ax

- 14 -

Thus:

dp. , (m -m ) 31* " " ̂ A B"13

dt S. Ax

dfoik= . (^ ^ o ^ - ^ - ^ o , ^ + - B_14

dt S. Ax /4k

^ k = _ (Pk^l Sk+1 ' Pk Sk) . (mk+l Vk+1 " mkVk)

dt Ax Ax

A ~ (Sk-H ~ Sk} , s, , ,. ,

+ Pk A^ (25T> !mk'Vk k

where p. and (-r*-.) correspond to values averaged over the h k

control volumes k.

B.2.3 Standard Simplified Form of the CVM-Equations

For practical reasons which will be presented later, the following

simplifying hypotheses are usually made:

a in the control volumes k (boundaries included), the v2

kinetic energy per unit mass y- i s negligible compared

to the specific internal energy u = c T

2 2 Y_ << c T -=> ^— << c T ="> i . • i. * c T. 2 v 2 p o,k - k p k

2 v —— << c T =*•*=> P i * P, 2 v Ko,k - *K in the control volumes k, the cross section is constant

and the contribution of the mass flow gradient to the

- 15

momemtum balance (equation A-25) is negligible in

comparison to that of the pressure gradient

Sk+1 - Sk

i"2k+r"<U) K< (pk+i sk+rpk sk )

Pk+i sk+ i A x fix

(Pk-,i s k , i ~Pk V A ( n w v k + i - mk V

fiX AX

•2 (1 - L.) Sk (pktfPk' + \ pk+l pk

Ax S, Ax k

Thus we obtain the standard simplified form of the CVM

equations:

• 9

dp̂ ̂ Vvi ) dt vk

d t - = \ — + ( x - 1 , ( * k B " 1 7

,1 1_. ^ k ( P k + r P k ) S k m2 p k + 1

pk ,5 , •• ,

dF Tx sT ——* (2Dr> 'mk' \ B'18

k h k

B.2.4 Remarks

It should be noted that the CVM equations B-13, B-14, B-15

are identical to the Fl-'/ equations B-10, B-ll, B-12 i.e.

the control volume method and the finite difference method

result in the same final set of equations provided that

the discretization schemes are comparable. Thus, there are

basically no fundamental differences between the 2 numerical

methods.

- 16 -

b The simplifying hypothesis of constant cross sectional

axea was only applied to the control volumes

The area changes do not appear explicitly in the

equations B-16 and B-17 relative to the control

volumes . Hence the standard simplified form B-16,

B-17, B-18 of the CVM equations is very practical,

particularly for overall plant simulation, as it

constitutes a convenient way to deal with the diffi­

cult handling of area changes: the flow channel is

discretisized in such a way that area changes only

take place in the control volumes

In order to distinguish between the 2 kinds of control

volumes, the flow channel is usually represented in

simulation scheme by a succession of plena (corre­

sponding to the control volumes ) and pipes

(corresponding to the control volumes ) as shown in

fig. 5.

B.3 Method of Characteristics (CHM)

The Method of Characteristics uses the fact that the basic

partial differential equationsB-4 to B-6 are of hyperbolic cha­

racter. This means that there exist lines in the t-x-plane,

the so called characteristics, where the dynamic variables of

a flow problem cannot be arbitrarily chosen, but are subject

to characteristic relations. The characteristic relations be­

come surprisingly simple for an isentropic flow in a constant

cross-section. It is convenient to chose the velocity of sound

c as a thermodynamic variable, pressure and density are then

given by:

- 17 -

+ *k~l p k - l

-4

"Vl Pk

I

*k+l p k * l

+

*k+l

I

plenum Pipe

F i g . 5

- 18 -

2K

° co

2 r-1

° co

The differential equations of the characteristics C in the

t-x plane are

C : §r = v + c B-20 dt —

and the characteristic relations are:

i 2 * J - v ± —^r c * constant an C B-21

+ The constancy of J , the so called Riemann-Invariants, allows

an explicit construction of the flow-field in the t-x-plane,

starting from the initial and boundary-conditions. The purely

geometrical construction of the characteristics in the x-t and

v-c planes is discussed in many textbooks on compressible fluid-

dynamics, e.g. in (1). The same method can also be put into

numerical form and results in very simple and fast computer

programs; but this is not commonly done. A detailed description

of the corresponding numerical method can be found in (2).

C. Experimental Investigation by the Shallow Water Analogy (SHW)

The local equations of motion B-l and B-3 for an isentropic flow

of e compressible fluid in two dimensions can be written as:

- 19 -

|| = - div (pv) C-1

a — (pv) = - div • (v p v) - grad p C-2

On the other hand, the flow of an ideal incompressible fluid

under the influence of gravity on a horizontal plane in two

dimensions can be described by the same set of equations, when

the following conditions are satisfied:

a) The depth of the fluid h must be small compared to

the wave length of the phenomena studied.

b) The vertical velocity must be small compared with

its horizontal component.

c) The vertical acceleration must be small compared with

gravity g.

Let x denote the two-dimensional position and h (x, t) the

time-dependent local depth of the fluid. The equations of

motion for the fluid can now be written in the form:

|| = - div (hv) C-3

l ^ L = - div (vhv) - V (f) C-4

Equations C-1, C-2 and C-3, C-4 are the same when the following

substitution is made:

p • a - h C-5

- 20 -

p = 2* h2 C-6

a is an arbitrary constant. From C-5 and C-6, the following

equation of state can be obtained by elimination of h:

p = k ' p2 - p 0 * {7~)K' K=2 c_7

o

This is exactly the equation of state for an ideal gas with

* = 2, e.g. the shallow water analogy models the motion of an

ideal gas with * = 2. A more detailed description of the ana­

logy can be found in (3).

D. Application to a Standard Problem

D.l The Standard Problem

A standard problem with a simple configuration (see below fig. 6)

is defined in order to allow a direct comparison between measure­

ments from the shallow water te.ble (see section 2) and numerical

results obtained with the different methods already presented in

part A.

p = 20 m2

p = 60 bar

V • 200 m3

10 m

S - 1 m2

15 m

Fig. 6 Geometry of the Standard Problem

- 21 -

The geometry of the standard problem has been chosen according

to 2 requirements:

the ratio of the volumes of the reservoir to the exit

area is representative of that corresponding to the

HHT-reactor inlet plenum,

the configuration is simple enough such that the water

table could be constructed.

The type of transients studied is the rapid depressurization of

the system initially filled with a stagnant ideal gas at a

uniform pressure of 60 bar. The time dependent pressure at the

exit is an input function given by measurements from the water

table (see fig. 9, measurement position nr. 1) .

D.2 Results

D.2.1 Shallow Water Analogy (SHW)

The analogy between shallow water flows and compressible flows

provides a convenient way to study experimentally the defined

standard problem. A water table was constructed according to

the geometry of the standard problem scaled down to 1 : 10

(see fig. 7).

The depressurization takes place when the slider is suddenly

opened, t'ms connecting the high pressure section (initially

at 60 bar) to the low pressure section (initially at 30 b&r).

The pressures are measured at 6 positions as shown in fig. 7.

- 22 -

p = 60 bar

1 m

Pressure^ measurement

• * •

. jp = 30 bar'

I

^ Slider.

LJ I

1.5 m

Fig. 7 Geometry of the Water Table

- 23 -

The following fig. 8 shows the water table with its measure­

ment equipment. A detailed description may be found in (4).

Fig. 8 The Water Table and the Measurement Equipment

The time dependent evolution of the pressures measured at the

6 positions is presented in fig. 9. The pressure at position 1

decreases from 60 bar to 35 bar in 4 ms. The expansion wave

runs along the pipe (position 2 and 3) toward the plenum and is

considerably damped out by the change in cross-sectional areas

between position 3 and 4. The pressure distribution in the

plenum remains astonishingly uniform* only slight differences

- 23 a -

Fig. 9 Experimental Results from the Shallow Water Analogy (SHW)

IK,

n,

ss.

s§.

45.

4f.

35.

m.

\

\ 1

1

POSITION M 1

1 1

\JT" Y i i

i

•—->

i

• ^ ^

55. _

S Sfl.

* m.

35. _

POSITION NR 2

T 1 1 r

J I I L

TINE IN MLLISECOND

•- 20. 4f. S». TIIC IN niLLISECOO

•. 2i. 4*. 60. THE IN niLLISECONO

I . 20. 4f.

TINE IN maiSECOND

0. 20. 4f. 60.

TIIC It. IflLUSECONO

65.

{ 55.

50. | _

45.

40.

1

1

POSITION NR 6

1 1

1 1

1

1

-

.

-2f. 0. 20. 40.

TINE IN MILLISECOND

- 24 -

between pressures at positions 4,5 and 6 are observed.

D.2.2 Finite Difference Method (FDM)

The finite difference equations B-10, B-11 and B-12 are derived

without any explicit hypothesis concerning the flow area. It is

however implicitly assumed in the 1-dimensional model that the

fractional rate of flow area change with respect to the flow 1 A ^

distance is small (- — << 1). This is not true for the sharp o AX

edged area change in the standard problem.

In order to resolve the difficulty, the discontinuous area change

can be treated as

the coupling of 2 pipes with different cross-sectional

areas,

or by approximating the flow area change by a continous

function S(x).

The standard system is divided into 2 distinct pipes with 2 2

cross sections S = 20 m and S = 1 m respectively and

the standard problem is solved by applying the equations

B-10, B-11 and B-12 to both. The following ideal con­

ditions are used at the junction of the 2 pipes:

m.. = m_

2 2

(h + f - ) ^ (h + | - ) 2 D-l

'l = S2

- 24 a -

Fig . 10 Numerical Results from the F in i t e Difference Method I

1

,.

1.

1.

1

1

POSITION NR I

1 1 i

i

• i

• i

• i

w^

I s

POSITION NR 2

T 1 1 r

J I I L -20. 0. 20. 40. 00. 80. -20. 0. 20. 40.

TIIC IN mLLISECONO TIRE IN RILLISECOND

Q SHU O FDR I

POSITION NR 3 _ POSITION NR 4

«0 1

55.

50.

45.

40.

35.

90.

1

"

1

1

1

1

1

1

1

^

^

_-

^

-20. 0. 20. 40.

TIRE IN niLLISECOND

-20. 0. 20. 40. 00.

Tift IN niLLISECOND

• SHU O FOR I

m.

99»

50.

45.

40.

»

POSITION NR 5

1 1 1

1 1 1

1

1

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- 25 -

The results obtained with the FDMl method are shown in fig. 10.

b 92D£iDH2H§_**f:5_9!*?59S-IE9!L*Il.

The sharp edged area change of the standard system is

approximated by a continuous linear function S (x) as

shown in fig. 11.

21 22

0.2 m

Fig. 11

- 26 -

A very fire discretization (10 in our calculation) of the part

of the plenum where the flow area is continuously varying is

therefore required in order to satisfy the condition

— — << 1. No coupling conditions are necessary as the system is

considered as a whole to which the equations B-10, B-11 and B-12

are applicable.

The results of the FDNII method are presented in fig. 12.

D.2.3 Control Volume Method (CVM)

The standard simplified form B-16, B-17 and B-18 of the control

volume equations are used. As previously mentioned, no special

care has to be made for the treatment of the area change if

the system were discretized in such a way that it occurs in a

control volume where the equations B-16 and B-17 are valid.

The number of control volumes considered is equal to the number

of axial zones used in the FDMI calculation.

Fig. 13 shows the results in comparison with the measurements

from the water table.

D-2.4 The Method of Characteristics

The method of characteristics is applied to the two cylindrical

parts of the standard problem. These two parts have been coupled

by use of the junction conditions D-l. The details of the com­

plete numerical algarithm have been described in (2). Fig. 14

shows the results of these calculations.

- 26 a -

Fig. 12 Numerical Results from the Finite Difference Method II

as.

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- 26 b -

Fig. 13 Numerical Results from the Control Volumes Method

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- 26 c -

Fig. 14 Numerical Results from the Method of Characteristics

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D. 3 Comparison

D.3.1 Comparison of the numerical methods FDH, CVK, CHM

The FDMI. CVM and CHM results are shown in fig. IS. The PDMII

results which correspond almost exactly to the IDMI results

are not presented.

At the positions 4, 5 and 6 in the plenum, only slight differen­

ces are observed whereas at positions 2 and 3 in the pipe, where

the fluid velocity is much greater, the differences are quite

noticeable. These differences were, however to be expected since:

the CHM method of characteristics makes use of an

isentropic flow model,

the CVM control volumes method (which results in the

same final set of equations as the PDM method as previously

mentioned in part B, section 2.4) was used in our calcu­

lations in its so called standard simplified form (see

part B, section 2.3) where the fluid kinetic energy and

the flow gradient were neglected in both the energy and

in the momentum balance respectively.

According to these additional simplifications introduced in the

CHM method and in the CVM method, the PDM should present the

best agreement with the measurements from the water table. This

is demonstrated by a comparison of the figures 10, 12, 13 "ind 14.

D.3.2 Comparison of the 1-D Compressible Plow Model with the

2-D Shallow Water Plow Model

The results obtained with the PDM method based on a 1-D compres­

sible flow model have already been compared, in figures 10 and

12, with the measurements from the water table.

- 27 a -

Fig. 15 Comparsion of the results obtained from three dif­ferent numerical methods with the same number of zones N = 25

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- 28 -

A very good agreement between the numerical results and measure­

ments was observed in the plenum thereby, confirming the validity

of the one-dimensional flow model for studies of rapid depressuri

zations of a reservoir.

However, in the vicinity of the sharp eged area change, the

2-dimensional effects (particularly the flow area contraction)

were very acute and consequently resulted in appreciable differen­

ces at positions 2, 3 and 4. Some of these 2-dimensional effects

(e.g. flow area contraction) could have been taken into account

in the 1-dimensional flow model using some refinements. Thus the

agreement between numerical results and measurements could be im­

proved, as shown in fig. 16, by introducing an empirical flow

area contraction ratio.

D.3.3 Influence of the number of discretization zones

With the FDM and CVM methods, a reduction in the number of dis­

cretization zones is desirable since it leads to a profitable

reduction in the computer running time. However, the influence

on the quality of the results has to be examined. For this pur­

pose, 2 CVM calculations with 25 and 3 zones respectively as

well as 2 FDM calculations with 25 and 5 zones respectively have

been run. The comparison of these results is presented in

fig. 17.

It is evident that informal-ion is less detailed if the number

of discretization zones is reduced. In the 3-zone CVM run,

only pressures at position 2 in the pipe and position 5 at the

middle of the plenum are computed. Nevertheless the pressure com­

puted at position 5 with fewer discretization zones (5 for FDM

and 3 for CVM) agrees favourably with that computed using 25

discretization zones for both FDM and CVM.

- 28 a -

Fig. 16 Numerical Results from the Finite Difference Method II with reduced cross-section of junction

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Fig. 17 Influence of the number of zones:

Fig. 17a: FDM I

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- 29 -

The depressurization wave is somewhat damped out at position nr. 2

if fewer discretization zones are used. This result is to be ex­

pected according to the FDM equation B-17 and to the greater

volume of fluid involved in a discretization zone.

E. Conclusions

E.l The 1-dimensional flow model

For the types of transients studied (depressurization of a plenum)

the 1-dimensional flow model seems to be quite satisfactory as

far as the depressurization of the plenum is concerned.

In the pipe, where 2-dimensional effects lead to appreciable

differences between numerical results and measurements, the 1-

dimensional flow model could be improved by introducing empiri­

cal requirements.

E.2 The different numerical methods

As previously emphasized in part B, section 2.4, no fundamental

differences occur between the FDM and CVM methods which would

result in the same final set of equations if the same discreti­

zation schemes were chosen.

A very good agreement between results obtained with the FDM,

CVM and CHM methods concerning the pressures in the plenum was

observed. However, differences did occur in the pipe where the

fluid velocity was greater due to the additional simplifications

introduced in the CHM method as well as in the standard simpli­

fied form of the CVM method.

Inspite of the isentropic flow hypothesis, the CHM method proved

to be very interesting due to its low computer costs.

- 30 -

The standard simplified form of the CVM method is particularly

convenient for an overall plant simulation code as it avoids

the difficulty of changes in flow area and is suitable for mo­

dular programming techniques.

E.3 The number of discretization zones

A reduction in the number of discretization zones does not affect

sensitively the results concerning the depressurization in the

plenum. However, in the exit pipe, the amplitude of the pressure

oscillations is considerably damped out.

- 31 -

The t r ans fo rma t ion of e q u a t i o n s B-4 t o B-6 i n t o B-7 t o B-9 _ • p v

by introduction of t he v a r i a b l e s p , m = pvS(x) and p =p+(K-l) *-=—

i s as fo l lows :

From A-4, A-5, A-7 and A-8 u can be expressed as:

(1)

pu = —fy and therefore It *•* J.

•«*r> - A <p*«-" T > - £ r

B-8 is obtained from the multiplication of B-5 with *-l and the

substitution of the new variables p and m

mation of equations B-4 and B-6 is obvious

substitution of the new variables p and m = ovS. The transfor-

The finite difference equations B-10 to B-12 are obtained by

application of the discretization method illustrated in Fig. 1

to the partial differential equations B-7 to B-9. Since the dy­

namical variables p, p and m are defined at different locations

in the discretization net, interpolation must be used in order

to calculate the other dependent variables: i . , p. (mv).

and p..

From A-4, A-5 and A-6

. ^ 1 2 K p 1 2 (2) 1 = 1 + T V = =- C + - V o 2 (c-1 p 2

is obtained. With help of (1) can be expressed in terms of p , p

and m :

2

1 - K=r-p0/P + (1"K) y b r 2 o)

- 32 -

p p and S are now interpolated at the junctions by

— Po,k+l * po tk - _ pk+l+pk ^- _ Sk+1 + Sk po,k = 2 ' pk " 2 ' 5k " 2

and i . is found by inserting these mean values into

— '2 K F£Ji + a-*) JS_ 2. (4)

o,k <-l 7^ 2 ( 5k Sk )

p can be expressed in p , P and m by solving (1)

2 j 2pS" P " Pn " <*-D 7^2 (5)

p is a zone-variable, p and p are already defined in the zone-

centers, m at the zone-centers must be interpolated by

(m) k = K

2 (6)

By introducing (6) into (5), p is found:

•2

Pk = Po,k " «'»' I^sf (7)

(mv). is defined as the value of mv at the zone centers. From k »2

mv = —- , (mv). can be found as: pS K

(mv). = — ~ - (8) k pk Sk

Two further junction variables are needed in B-12: p and (mv). .

- 33 -

These are directly formed as ari thine trie mem of the adjacent

zone variables p. and (m v).:

Pk + pk 1 — <mv\, + tmv)

pk= j - ' (mv)k — - Inv),. = S__̂ ^-± (9)

Finally (r̂ r-) is the local value of the expression *r- at the 2Dh k 2Dh

junction k and q. is the mean of the heat-input per unit volume

and time at the zone k.

- 34 -

References

(1) G. Rudinger,

Wave Diagrams for nonsteady Flow in Ducts,

D. Van Nostrand Company, New York, 1955

(2) H. Weber,

Anwendung der Charakteristiken-Hethode fur die Kreislauf-

dynamik,

Swiss Federal Institute for Reactor Research, Wiirenlingen,

Switzerland,

Report TM-ST-392, 1976

(3) P.A. Thompson,

Compressible-Fluid Dynamics,

McGraw-Hill, New York, 1972

Chapter 11

(4) H. Weber,

StrSmungsversuche mit dem Wassermodell:

Beschreibung der Versuchseinrichtung,

Swiss Federal Institute for Reactor Research,

WUrenlingen, Switzerland

Report TM-ST-421, 1976

(5) HHT-Project

Referenzanlage, Phase IB

Report HHT-27, HRB-BA1671

October 1977

(6) C.F. McDonald,

Large Closed-Cycle Gas Turbine Plant

GA-A 14311

General Atomic company,

May 1977

- 35 -

(7) Gas turbine HTGR

A technology assessment

Report NUS-3041, NUS Corporation Maryland

October 1977

(8) A. Tiberini

Das dynamische Verhalten eines gasgekühlten

schnellen Brutreaktors mit direktem Gasturbinen­

kreislauf, dargestellt am Beispiel des Rohrbruch-

Unfalles in einer 1000 MWe-Anlage mit Rekuperator.

EIR-Bericht Nr. 263 und Dissertation ETH-Zürich Nr. 5329

Juni 1974

(9) M. Waloch

Anlagenstörfalldynamik von Hochtemperaturreaktoren

mit direktem Gasturbinenkreislauf

Institut für Dampf- u. Gasturbinen

RWTH - Aachen, 1977

(10) J.F. Dupont, R. Jeanmonod, H.U. Frutschi

TUGSIM-10, A Computer Code for Transient Analysis

of Closed Gas Turbine Cycles and Specific Applications

Nuclear Engineering and Design 40 (1977) p.421-430.

(11) G. Krey

Das dynamische Verhalten von einwelligen geschlossenen

Dampfturbinen,

Institut für Strömungsmaschinen, Technische Universität

Hannover,

Bericht 288/74, 1974.

- 36 -

(12) P. Quell,

Die Bedeutung von Bruchstorfallen bei Kernkraftwerken mit

Hochtemperaturreaktor und Heliumturbinenkreislauf in

nicht-integrierter Bauweise

KFA-Jiilich, Institut fur Reaktorentwicklung

Bericht KFA Nr. 1244 und Dissertation RWTH-Aachen

October 1975

(13) J. Dean, G. Preinreich, G. Soubelet,

Control and Safety Studies for an HTR Gas Turbine System.

International Conference on Nuclear Gas Turbines

BNES, London (1970), Paper No. 10

(14) J.F. Dupont, G. Cina, M. Dang,

PLAYGAS, a computer Code for the Transient Analysis

of Nuclear Gas Turbine Power Plants

First European Nuclear Conference, April 1975, Paris

and EIR-Bericht Nr. 284.