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Introduction to Loop Heat Pipes Jentung Ku NASA/ Goddard Space Flight Center GSFC· 2015 Introduction to LHP - Ku 2015 TFAWS https://ntrs.nasa.gov/search.jsp?R=20150018090 2018-06-08T02:20:37+00:00Z
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Page 1: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

Introduction to Loop Heat Pipesp p

Jentung KugNASA/ Goddard Space Flight Center

GSFC· 2015

Introduction to LHP - Ku 2015 TFAWS

https://ntrs.nasa.gov/search.jsp?R=20150018090 2018-06-08T02:20:37+00:00Z

Page 2: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

Outline

• From Heat Pipe to Loop Heat Pipe (and Capillary Pumped Loop)

• LHP Operating PrinciplesLHP Operating Principles• LHP Components Sizing and Fluid Inventory• LHP Operating Temperature Control• LHP Start-up• LHP Shutdown • LHP Analytical Modeling• LHP Analytical Modeling• Recent LHP Technology Developments

Introduction to LHP - Ku 2015 TFAWS 2

Page 3: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

From Heat Pipe to Loop Heat PipeFrom Heat Pipe to Loop Heat Pipe and Capillary Pumped Loop

Introduction to LHP - Ku 2015 TFAWS 3

Page 4: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

Heat Pipes - Heat Transport Limit• For proper heat pipe operation, the

total pressure drop must not exceed its capillary pressure head .

Ptot ≤ Pcap,max

Ptot = Pvap+ Pliq + Pg

Liquid Flow

Heat SinkHeat Source

wall

Le LaLc

Pcap,max = cos/Rp

• Heat Transport Limit– (QL)max = QmaxLeff

– Leff = 0.5 Le + La + 0.5 Lc

wallLiquid Flow

Evaporator CondenserAdiabaticS ti

Vapor Flow

VaporVapor

eff e a c

– (QL)max measured in watt-inches or watt-meters

• Capillary pressure head:

P 1/ R

Section SectionSection

LiquidPressure DropPr

essu

re CapillaryPressure

VaporPressure Drop

Liquid

Li id

Pcap 1/ Rp

• Liquid pressure drop:

Pliq 1/ Rp2

A ti l di i t f

Le La Lc

LiquidNo Gravity Force

Adverse Gravity Force

• An optimal pore radius exists for maximum heat transport.

• Limited heat transport capability

• Limited pumping head against gravity

Introduction to LHP - Ku 2015 TFAWS 4

Distance

b) Vapor and liquid pressure distributions

p p g g g y

Page 5: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

EvaporatorWickHeat In

Constant Conductance Capillary Pumped Loop

S

Vapor Out

Heat Out

Liquid In

Vapor

SubcoolingLiquid Leg Condenser

Duct

Heat Out

High VelocityVapor PlusLiquid WallFilVapor

Bubble

Liquid“Slug”

Film

Flow ForcesPredominateSurface Tension

Forces Predominate

• Wicks are present only in the evaporator, and wick pores can be made small.• Smooth tubes are used for rest of the loop, and can be separately sized to

reduce pressure drops.

Introduction to LHP - Ku 2015 TFAWS

• Vapor and liquid flow in the same direction instead of countercurrent flows.• Operating temperature varies with heat load and/or sink temperature.

5

Page 6: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

Variable Conductance Capillary Pumped Loop Reservoir

Evaporator

Liquid Line

Vapor Line

• The reservoir stores excess liquid and controls the loop operating

Condenser

The reservoir stores excess liquid and controls the loop operating temperature.

• The operating temperature can be tightly controlled with small heater power.

• The loop can be easily modified or expanded with reservoir re-sizing.• Pre-conditioning is required for start-up.• Evaporator cannot tolerate vapor presence, may be prone to deprime

Introduction to LHP - Ku 2015 TFAWS 6

during start-up.• Polyethylene wick with pore sizes ~ 20 µm

Page 7: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

Capillary Two-Phase Thermal DevicesHeat In

Reservoir

Evaporator

ne

Evaporator

ReservoirHeat In

Liquid Line

Vapor Line

Condenser/Subcooler

Vapo

r Lin

Liqu

id L

ine Heat

In/Out

Condenser

Line

Heat Out

Wick Structure

Container Wall QOUTQIN

Liquid FlowVapor Flow

CondensationEvaporization

Introduction to LHP - Ku 2015 TFAWS 7

q

Page 8: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

CPL and LHP Flight Applications – NASA Spacecraft

TERRA 6 CP HST/SM - 3B; 1 CPLLaunched Feb 2002

TERRA, 6 CPLsLaunched Dec 1999

AURA, 5 LHPsLaunched July 2004

Introduction to LHP - Ku 2015 TFAWS 8

ICESat, 2 LHPsLaunched Jan 2003

SWIFT, 2 LHPsLaunched Nov 2004

GOES N-Q, 5 LHPs eachLaunched 2006

Page 9: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

CPL and LHP Flight Applications – NASA Spacecraft

SWOT, 4 LHPsTo be launched

GOES R-U, 4 LHPs eachTo be launched

ICESat-2, 1 LHPTo be launched

• LHPs are also used on many DOD spacecraft and commercial satellites.

Introduction to LHP - Ku 2015 TFAWS 9

Page 10: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

Introduction to Loop Heat Pipes

Introduction to LHP - Ku 2015 TFAWS 10

Page 11: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

Schematic of an LHP

Primary wick

ArteriesCompensationChamber Evaporator

BayonetA

Primary wick Secondary wick

Secondary wick

Bayonet

Vapor GroovesVapor line

Vapor grooves

Liquidline

A

y

Section A-A

Condenser

• Main design features− The reservoir (compensation chamber or CC) forms an integral part of the evaporator assemblyintegral part of the evaporator assembly.− A primary wick with fine pore sizes provides the pumping force.

A secondar ick connects the CC and e aporator

Introduction to LHP - Ku 2015 TFAWS

− A secondary wick connects the CC and evaporator, providing liquid supply.

11

Page 12: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

Main Characteristics of LHPHeat In

Vapo

r Lin

e

uid

Line

Evaporator

Heat In/Out

Reservoir Heat In

Condenser/Subcooler

V

Liqu

Heat Out

• High pumping capability– Metal wicks with ~ 1 micron pores– 35 kPa pressure head with ammonia (~ 4 meters in one-G)

Heat Out

p ( )• Robust operation

– Vapor tolerant: secondary wick provides liquid from CC to evaporator• Reservoir is plumbed in line with the flow circulation.

– Operating temperature depends on heat load, sink temperature, and surrounding temperature.

– External power is required for temperature control.Limited growth potential

Introduction to LHP - Ku 2015 TFAWS

– Limited growth potential• Single evaporator most common

12

Page 13: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

• The total pressure drop in the loop is the sum of viscous pressure drops in LHP

LHP Operating Principles – Pressure BalanceThe total pressure drop in the loop is the sum of viscous pressure drops in LHP components, plus any pressure drop due to body forces:Ptot = Pgroove + Pvap + Pcond + Pliq + Pwick + Pg (1)

• The capillary pressure rise across the wick meniscus: Pcap = 2 cos /R (2)

• The maximum capillary pressure rise that the wick can sustain:• The maximum capillary pressure rise that the wick can sustain: Pcap, max = 2 cos /rp (3)

rp= radius of the largest pore in the wickp g p

• The meniscus will adjust it radius of curvature so that the capillary pressure rise matches the total pressure drop which is a function of the operating condition: P P (4)Pcap = Ptot (4)

• The following relation must be satisfied at all times for proper LHP operation:Ptot Pcap max (5)

Introduction to LHP - Ku 2015 TFAWS

Ptot Pcap, max (5)

13

Page 14: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

Pressure Profile in Gravity-Neutral LHP Operation Capillary Force Driven

P1

Vapor Channel

Primary WickSecondary

WickBayonet

2

6

1 P2 P3 P4P5 P6su

reReservoir Evaporator1 7

Pres

s

P

Vapor Line

Liquid Line

Condenser

Location

P7

77 (Liquid)(Liquid)

35 4

• Evaporator core is considered part of reservoir.• P6 is the reservoir saturation pressure.• All other pressures are governed by P6

Introduction to LHP - Ku 2015 TFAWS

p g y 6• All pressure drops are viscous pressure drops.

14

11wickwick (Vapor)(Vapor)

Page 15: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

Thermodynamic Constraints in LHP Operation (1)• For the working fluid in a saturation state there is a one-to-one• For the working fluid in a saturation state, there is a one-to-one

correspondence between the saturation temperature and the saturation pressure.

• There are three LHP elements where the working fluid exists in a two-phase state, i.e. evaporator, condenser and reservoir.

• There is a thermodynamic constraint between any two of the above-mentioned three elements, i.e. the pressure drop and the temperature drop between any two elements aretemperature drop between any two elements are thermodynamically linked. E.G.

PE – Pcc = (dP/dT) (TE – Tcc)

• The derivative dP/dT can be related to physical properties of the working fluid by the Clausius-Clapeyron equation:

Introduction to LHP - Ku 2015 TFAWS

dP/dT = / (Tcc v)

15

Page 16: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

Thermodynamic Constraints in LHP Operation (2)

Vapor Channel

Primary Wick

Secondary Wick

Bayonet

2

6

Saturation Curve

Reservoir Evaporator

Li id1 7

ress

ure P4

P1

P6

6

1

4

Vapor Line

Liquid Line

Condenser

35

Pr

T4 T1

VaporLiquid

T6

PE – Pcond = (dP/dT) (TE – Tcond)

35 4 Temperature

Pcond – Pcc = (dP/dT) (Tcond – Tcc)

PE – Pcc = (dP/dT) (TE – Tcc)

Introduction to LHP - Ku 2015 TFAWS 16

• Gravity affects the pressure drop, and hence the temperature difference.

Page 17: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

LHP Operating Principles – Energy BalanceReservoir

e

Evaporator

ReservoirQIN mQsub

Q

Condenser/Subcooler

Vapo

r Lin

e

Liqu

id L

ine

QRA

Qleak

QLA

QC,2ΦQC,1Φ

m

),,( ,2,, wallccoutc TLmfT

TDLmTfT

LEIN QQQ

CCECCEL TTGQ , ambLLLLoutcIN TDLmTfT ,,,,,

INCCPsub TTCmQ mQE

)(2 ,2,2,2, wallcCCcccc TThLDmQ

Introduction to LHP - Ku 2015 TFAWS 17

0 RAsubleak QQQ

Page 18: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

Simplified LHP Thermal NetworkReservoir Heat In

Condenser/Subcooler

Vap

or L

ine

Liqu

id L

ine

Evaporator

Heat In/Out

ambT

Q eQ

cceQ ,

Heat Out

,

l

lT

hmcc

ccT

hm, ,eT

ehm

accQ , eQ

CompensationChamber

Evaporator

0l

lq

Tcc

ccq 1eq

hmhm

avQ ,

ambT

ambT

alQ ,

1

,

v

satv

v

qTThm

0

,

c

satc

c

qTThm

0

,

sc

sc

sc

qT

hm

InactiveCondenser(Subcooler)

ActiveCondenser

Introduction to LHP - Ku 2015 TFAWS sinkT

scQ ,

sinkT

sscQ , Vapor LineLiquid Line

18

Page 19: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

LHP Reservoir Sizing and Fluid Inventory

• The fluid inventory must satisfy the following relation under the cold start-up/operation ( > 0):

or L

ine

d Li

ne

Evaporator

Heat In/Out

ReservoirHeat In

M = l,c (Vloop + Vcc )+ v,c (1- )Vcc

Vloop = Loop volume excluding CCCondenser/Subcooler

Vapo

Liqu

id

Heat Out

• The fluid inventory must also satisfy the following relation under the hot operating condition ( > 0):M = l h [Vliq +Vpw +Vsw +(1-) Vcc] + v h (Vgr + Vvap +Vcon + Vcc )M l,h [Vliq Vpw Vsw (1 ) Vcc] v,h (Vgr Vvap Vcon Vcc )

• The values of and , selected at the designer’s discretion, determine Vcc and M.cc

• The loop must contain all liquid volume at the maximum non-operating temperature:

Introduction to LHP - Ku 2015 TFAWS

M l, max (Vloop + Vcc)

19

Page 20: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

ICESat-2 ATLAS LHP Charge Analysis 15% Fill in Cold Case15% Fill in Cold Case

• Charge to maintain 15% CC fill fraction in the cold case startup conditions• LHP requires 193.4 grams of ammonia

Volume Cold Start-up Non-Operating Case Operating Hot Caseliquid liquid vapor liquid liquid vapor liquid liquid vapor

fraction temp dens dens mass fraction temp dens dens mass fraction temp dens dens massin3 cc in3 cc K gm/cc gm/cc gms K gm/cc gm/cc gms K gm/cc gm/cc gms

Evaporator (vapor) 0.43 7.1 0.4 7.1 1.00 268 0.65 0.0029 4.6 1.00 333 0.54 0.0213 3.8 0.00 313 0.57 0.0126 0.1Evaporator (liquid) 4 67 76 5 4 7 76 5 1 00 268 0 65 0 0029 49 5 1 00 333 0 54 0 0213 41 1 1 00 313 0 57 0 0126 43 6Evaporator (liquid) 4.67 76.5 4.7 76.5 1.00 268 0.65 0.0029 49.5 1.00 333 0.54 0.0213 41.1 1.00 313 0.57 0.0126 43.6Liquid Core 0.69 11.2 0.7 11.2 1.00 268 0.65 0.0029 7.3 1.00 333 0.54 0.0213 6.0 1.00 313 0.57 0.0126 6.4Vapor transport line 1.28 21.0 1.3 21.0 1.00 233 0.69 0.0007 14.0 1.00 333 0.54 0.0213 11.3 0.00 313 0.57 0.0126 0.3Condenser 4.92 80.6 4.9 80.6 1.00 233 0.69 0.0007 55.4 1.00 333 0.54 0.0213 43.3 0.12 313 0.57 0.0126 6.2Liquid Transport Line 2.00 32.8 2.0 32.8 1.00 233 0.69 0.0007 21.9 1.00 333 0.54 0.0213 17.6 1.00 313 0.57 0.0126 18.7Hydro-accumulator Wicks Liquid 0.24 3.9 0.2 3.9 1.00 268 0.65 0.0029 2.5 1.00 333 0.54 0.0213 2.1 1.00 313 0.57 0.0126 2.2Hydro-accumulator Free Volume 23.50 385.1 23.5 385.1 0.15 268 0.65 0.0029 38.3 0.302 333 0.54 0.0213 68.2 0.518 313 0.57 0.0126 116.0

TOTAL 37 72 618 27 37 7 618 3 193 4 193 4 193 4

– 15% required reservoir liquid fraction at cold startup (β = 0.15)– Design has 70% void volume in hot non-operational (processing) case at 60C

TOTAL 37.72 618.27 37.7 618.3 193.4 193.4 193.4

g p (p g)– 51.8% max fill at hot operating condition (α = 0.482)

Typical values: 0.15 ( 0.85 liquid fraction)

Introduction to LHP - Ku 2015 TFAWS

0.15 (0.15 liquid fraction)

20

Page 21: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

LHP Operating Temperature• The LHP operating temperature is governed by the CC saturationThe LHP operating temperature is governed by the CC saturation

temperature.• The CC temperature is a function of

– Evaporator powerEvaporator power– Condenser sink temperature– Ambient temperature– Evaporator/CC assembly designEvaporator/CC assembly design

• As the operating condition changes, the CC temperature will change during the transient, but eventually reaches a new steady temperature.

empe

ratu

re

T1

T2

12 5or

Lin

eEvaporator

ReservoirQIN m

QRAC

C T

e

T3

T5

3

5

Condenser/Subcooler

Vapo

Liqu

id

Line

m

Introduction to LHP - Ku 2015 TFAWS

Net Evaporator PowerQ2 Q3 Q5QC,2ΦQSC

21

Page 22: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

LHP Operating TemperatureNo Active Control of CC Temperature

e

T1 1Line

Evaporator

ReservoirQIN m

QRA

CC

Tem

pera

ture

T2

T5

1

25Condenser/Subcooler

Vapo

r L

Liqu

id

Line

QQ

m

-Qsub QleakCC, Tcc

C

T3

Q2 Q3 Q5

3QC,2ΦQC,1Φ

Qleak – Qsub = 0

Net Evaporator Power

• For a well insulated CC, Tcc is determined by energy balance between heat leak and liquid subcooling.

Introduction to LHP - Ku 2015 TFAWS

• Tcc changes with the evaporator power, condenser sink temperature, and ambient temperature.

22

Page 23: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

Effect of Sink Temperature on CC Temperature -Theory

ratu

reC

C T

empe

r

T2min

T1min

Net Evaporator Power

Q2 Q1

1min

Introduction to LHP - Ku 2015 TFAWS

Net Evaporator Power

23

Page 24: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

Ground Test Results of Thermacore miniLHP at Various Sink Temperatures

Operating Temperature vs Power (New Chiller, Evaporator above Condenser by 0.25")

330

310

320

(K)

Heater on large TM (Tsink = 293K)

Heater on large TM(Tsink = 273K)

Heater on large TM(Tsink = 253K)

Heater on Evap.(Tsink = 293K)

Heater on Evap.(Tsink = 273K)

300

310

ting

Tem

pera

ture

Heater on Evap.(Tsink = 253K)

280

290

Ope

rat

2700 20 40 60 80 100 120

Power (W )

Introduction to LHP - Ku 2015 TFAWS 24

Page 25: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

LHP Operating TemperatureCC Temperature Controlled at Tset

atur

e

Natural Operating Temperature

Natural Operating Temperature

Q Q

Qcc

CC

Tem

pera

Fixed Operating TemperatureTsetTset

-Qsub QleakCC, Tcc≡Tset

C li Q Q

Heating Required

Qcc = Qsub - Qleak

Qleak - Qsub + Qcc = 0

• CC is cold biased, and electrical heaters are commonly used to maintain Tcc at Tset.O ll th l d t d

Power InputCooling Req’d

QLow QHighQcc Qsub Qleak

• Overall thermal conductance decreases.• Qcc varies with Qsc, which in turns varies with evaporator power, condenser sink

temperature, ambient temperature and number of coupling blocks.• Qcc can be large under certain operating conditions.

Introduction to LHP - Ku 2015 TFAWS

• Electrical heaters can only provide heating, not cooling, to CC.

25

Page 26: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

LHP Temperature Control Methods

• All methods involve cold-biasing the CC and use external heat source to maintain CC temperature– Electric heater on CC only (Aura TES, GOES-R GLM)y ( , )– Electric heater on CC and coupling blocks placed between

vapor and liquid lines (ICESat GLAS)– Electric heater on CC and VCHP connecting the evaporatorElectric heater on CC and VCHP connecting the evaporator

and liquid line (Swift BAT)– Pressure regulator on the vapor line with a bypass to liquid

line (AMS)line (AMS)– TEC on CC with thermal strap connecting to the evaporator

(heating and active cooling) – no electric heater (ST8)Heat exchanger and separate subcooler (GOES R ABI– Heat exchanger and separate subcooler (GOES-R ABI, ICESat-2 ATLAS)

Introduction to LHP - Ku 2015 TFAWS 26

Page 27: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

LHP Operating Temperature ControlElectric Heater on CC

Reservoir Heat In

QCC

Q Q

Qcc

Vapo

r Lin

e

Liqu

id L

ine

Evaporator

Heat In/Out

-Qsub QleakCC, Tcc≡Tset

Condenser/Subcooler

L

Heat OutQcc = Qsub - Qleak

Qleak - Qsub + Qcc = 0

• The electrical heater attached to the CC provides the necessary

Qcc Qsub Qleak

control heater power to the CC.• Advantages: simplicity, direct heating• Disadvantage: required control heater power could be large.

Introduction to LHP - Ku 2015 TFAWS 27

Page 28: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

EOS-Aura Tropospheric Emission Spectrometer (TES) Instrument Loop Heat Pipe Layout

SIGNAL CHAIN/ LASER HEAD ASSEMBLYLHP EVAPORATOR

MECHANICAL COOLER BLHP EVAPORATOR

MECHANICAL COOLER ALHP EVAPORATOR

IEM LHP EVAPORATOR

MECHANICAL COOLER ELECTRONICS LHP EVAPORATOR

Introduction to LHP - Ku 2015 TFAWS

EVAPORATOR

28

Page 29: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

• CCHPs and LHPs manage equipment

Tropospheric Emission Spectrometer (TES)CCHPs and LHPs manage equipment power dissipation from: 2 Mechanical Cooler Compressors Cooler electronics Signal Chain and Laser Head

l t ig

electronics Integrated Electronics Module (IEM)

Cooler Electronics B

Instrument Electronics Module

Introduction to LHP - Ku 2015 TFAWS 29

Cooler Electronics A

Page 30: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

EOS-Aura TES Components Thermal Performance

Introduction to LHP - Ku 2015 TFAWS 30

Page 31: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

LHP Operating Temperature ControlUse Coupling Blocks

Vapor Line

QE

QCC

Q Q

Qcc

Liquid Line

EvaporatorReservoir

Coupling Blocks

-Qsub QleakCC, Tcc≡Tset

Condenser

Qcc = Qsub - Qleak

Qleak - Qsub + Qcc = 0

• The coupling blocks serve as a heat exchanger which transfers heat from the vapor line to the liquid line.

QSubQC

Qcc Qsub Qleak

– Re-distribution of LHP internal heat• The reduction of liquid subcooling, Qsub, leads to reduced Qcc.• The contact area of coupling blocks is determined by the LHP hot

operational condition; the CC heater is then sized to accommodate the

Introduction to LHP - Ku 2015 TFAWS

operational condition; the CC heater is then sized to accommodate the worst subcooling condition.

31

Page 32: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

LHP Operating Temperature ControlUse Coupling Blocks

Vapor Line

QE

QCC

ture

Natural Operating Temperature

Natural Operating Temperature

Liquid Line

EvaporatorReservoir

Coupling Blocks C

C T

empe

rat

Fixed Operating TemperatureTsetTset

Condenser

Q Q

Heating Required

• Advantages– Easy to implement

QSCQC

Power InputCooling Req’d

QLow QHigh

– Efficient in reducing CC control heater power• Disadvantages

– Increases the natural operating temperature at low and high powers

Introduction to LHP - Ku 2015 TFAWS

– May add difficulty to low power start-up– May still require high CC control heater power under the cold condition.

32

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LHPs on ICESat• GLAS has high powered lasers to measure• GLAS has high powered lasers to measure

polar ice thickness• First known application of a two-phase loop

to a laser• 2 LHPs; Laser altimeter and power• 2 LHPs; Laser altimeter and power

electronics – Propylene LHPs

• Launched January, 2003B th LHP f ll t d• Both LHPs successfully turned on

• Very tight temperature control ~ 0.2 oC

Radiator

High Power Lasers

Radiator

Loop HeatPipe

Introduction to LHP - Ku 2015 TFAWS 33

Page 34: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

Coupling Blocks on ICESat GLAS LHPs

• There are eight coupling blocks between the vapor and liquid lines for each LHP.– Liquid subcooling is reduced by about one half.

• The ICESat spacecraft was launched in January 2003.• Both LHPs have been working very well.

Introduction to LHP - Ku 2015 TFAWS

g y

34

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GLAS Laser Temperatures• LLHP active control is finer than can be measured in the laser

GLAS CLHP Transient Data 02/20/03 (Laser Turn-on Turn off warmup heaters all

• LLHP active control is finer than can be measured in the laser telemetry when the LHP is at full 110 W of power

GLAS CLHP Transient Data 02/20/03 (Laser Turn-on, Turn off warmup heaters, all components powered)

20

30

0

10

0:00

.8

5:01

.8

0:04

.8

5:06

.8

0:08

.8

5:09

.8

0:12

.8

5:13

.8

0:16

.8

5:17

.8

0:20

.8

5:24

.8

0:25

.8

5:28

.8

0:29

.8

5:33

.8

0:35

.8

5:38

.8

0:41

.8

5:42

.8

0:45

.8

5:47

.8

0:49

.8

5:50

.8

0:53

.8

5:54

.8

0:57

.8

5:58

.8

1:01

.8

6:03

.8

1:05

.8

6:06

.8

1:09

.8

6:10

.8

1:13

.8

6:14

.8

ure

(°C

)

-30

-20

-10

2003

/051

-15:

00

2003

/051

-15:

15

2003

/051

-15:

30

2003

/051

-15:

45

2003

/051

-16:

00

2003

/051

-16:

15

2003

/051

-16:

30

2003

/051

-16:

45

2003

/051

-17:

00

2003

/051

-17:

15

2003

/051

-17:

30

2003

/051

-17:

45

2003

/051

-18:

00

2003

/051

-18:

15

2003

/051

-18:

30

2003

/051

-18:

45

2003

/051

-19:

00

2003

/051

-19:

15

2003

/051

-19:

30

2003

/051

-19:

45

2003

/051

-20:

00

2003

/051

-20:

15

2003

/051

-20:

30

2003

/051

-20:

45

2003

/051

-21:

00

2003

/051

-21:

15

2003

/051

-21:

30

2003

/051

-21:

45

2003

/051

-22:

0

2003

/051

-22:

1 6

2003

/051

-22:

3

2003

/051

-22:

4 6

2003

/051

-23:

0

2003

/051

-23:

1 6

2003

/051

-23:

3

2003

/051

-23:

4 6

Tem

pera

tu

-50

-40

Time (s)

Introduction to LHP - Ku 2015 TFAWS

TGLLHP2LLCCT TGLLHP2RADT TGLLHP2VLT TGLLHP2EVAPT

35

Page 36: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

LHP Operating Temperature ControlUse VCHP to Couple Evaporator and Liquid Line

QE

EvaporatorReservoirQCC

Q Q

Qcc

Vapo

r Lin

e

Liquid Line

VCHP-Qsub Qleak

CC, Tcc≡Tset

Condenser

Liquid Line

Qcc = Qsub - Qleak

Qleak - Qsub + Qcc = 0

• The VCHP transmits heat from the evaporator to the liquid line when the t li id i t ld d i th t f li id b li Q

QSCQC

Qcc Qsub Qleak

return liquid is too cold, reducing the amount of liquid subcooling, Qsub.– The required CC control heater power Qcc is reduced.

• The VCHP is shut down when more subcooling is needed.

Introduction to LHP - Ku 2015 TFAWS 36

Page 37: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

LHP Operating Temperature ControlUse VCHP to Couple Evaporator and Liquid Line

atur

e

Natural Operating Temperature

Natural Operating Temperature

QE

EvaporatorReservoirQCC

CC

Tem

pera

Fixed Operating TemperatureTsetTset

Vapo

r Lin

e

Liquid Line

VCHP

Q Q

Heating Required

Condenser

• Advantage– Active control of heating the liquid line versus passive heating when

Power InputCooling Req’d

QLow QHighQSCQC

g q p gcompared to the coupling blocks

• Disadvantages– Needs a VCHP, which may not be ground testable.

N d dditi l t l d i f th VCHP

Introduction to LHP - Ku 2015 TFAWS

– Needs an additional control device for the VCHP.– VCHP reservoir requires cold biasing.

37

Page 38: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

LHPs on SWIFT BAT• Burst Alert Telescope, a gamma ray detector array, is one of three p , g y y,

instruments on Swift .• Launched: November 20 , 2004 • Detector array has 8 CCHPs for isothermalization and transfer of 253 W

to dual, redundant, LHPs located on each side.

ShieldLHP 2 Condenser

DetectorArray

Shield

LHP 1 C d

LiquidLine 2

LiquidLine 1

LHP

ArrayLHP 1 Condenser VaporLine 2

CompensationChamber 2

Vapor Line 1

LHP evaporator

CompensationChamber 1

LHP 1 Evaporator

LHP 2 Evaporator

V Li 1

Introduction to LHP - Ku 2015 TFAWS

CompensationChamberRadiator

For both loops

p

Liquid Line 1 Liquid Line 2 Vapor Line 2

Vapor Line 1

38

Page 39: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

Swift BAT LHP Evaporator Assembly

Titanium bracket support of hydro-accumulator

G-10 washers for thermal isolation

pp y

Saddle soldered to VCHP

Aluminum clamps for VCHP

CCHPs attached to evaporatorsaddle with Eccobond G-10 washers for

th l i l tiSaddle attached to evaporatorpump with Eccobond

thermal isolation

Heat exchanger swaged over VCHP condenser

Introduction to LHP - Ku 2015 TFAWS 39

Titanium support bracket for VCHP reservoir

Page 40: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

BAT Flight Data Both LHPs Day 013 (1/13/2005)Nominal Operation

Loop 0 CC Loop 0 Evap (A1) Loop 0 Vapor @ Cond Loop 0 Lower Cond Loop 0 Cond OutletDAP Loop 1 Evap (B1) Loop 1 Vapor @ Cond Loop 1 Lower Cond Loop 1 Cond Outlet

10

20

p p ( ) p p @ p p

-10

0

ratu

re (C

)

-30

-20

Tem

per

-50

-40

0:00 1:00 2:00 3:00 4:00 5:00 6:00 7:00 8:00 9:00 10:00 11:00 12:00

• Temperature fluctuations of detectors < 0.4 0C• Frequent spacecraft slews have no noticeable effect on LHP operation.

UTC Time (Hr:min)

Introduction to LHP - Ku 2015 TFAWS

• Flight results verify satisfactory operation of dual LHPs for tight temperature control.

40

Page 41: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

LHP Operating Temperature ControlUse Heat Exchanger and Separate Subcooler

Vapor Line

QE

EvaporatorReservoir

QCCQcc

id L

ine Heat

Exchanger

-Qsub QleakCC, Tcc≡Tset

Condenser

Liqu

i

Subcooler

Qcc = Qsub - Qleak

Qleak - Qsub + Qcc = 0

• The subcooler is separated from the condenser.

Th li id li i l d ith th li th h h t h h

QcQsub

Qcc Qsub Qleak

• The liquid line is coupled with the vapor line through a heat exchanger, where liquid is allowed to vaporize. The liquid line then enters the subcooler.

• With proper sizing, the heat exchanger will take away most of the subcooling, and the subcooler will provide slightly subcooled liquid to the CC

Introduction to LHP - Ku 2015 TFAWS

the subcooler will provide slightly subcooled liquid to the CC.• Results of TV testing of ABI LHPs indicate that the design meets the LHP

temperature control and CC control heater power requirements.41

Page 42: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

LHP Operating TemperatureUse Heat Exchanger and Separate Subcooler

atur

e

Natural Operating Temperature

Natural Operating Temperature

Vapor Line

QE

EvaporatorReservoir

QCC

CC

Tem

pera

Fixed Operating TemperatureTsetTset

uid

Line Heat

Exchanger

Q Q

Heating RequiredCondenser

Liqu Subcooler

• Advantages– The natural operating temperature will be closer to Tset for heat loads

Power InputCooling Req’d

QLow QHighQ

CQsub

p g p setbetween QLow and QHigh.

– The CC control heat power is reduced significantly.• Disadvantages

– Needs a separate subcooler

Introduction to LHP - Ku 2015 TFAWS

Needs a separate subcooler.– Needs a longer liquid line, which imposes a higher frictional pressure drop.

42

Page 43: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

GOES-R ABI Radiator/LHP Assembly System Architecture

Evaporator Assemblies (2)

TransportLines

HeatExchangers (2)

S b l R iSub-cooler Region(Condenser-like linesembedded in Panel)

TransportLines

Introduction to LHP - Ku 2015 TFAWS 43

Page 44: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

LHP Operating Temperature ControlUse Pressure Regulator and Vapor Bypass

QE

Evaporator

ReservoirQCCQcc

Line

quid

Lin

e QPressure Regulator

Vapor Bypass

-Qsub QleakCC, Tcc≡Tset

Condenser

Vapo

r LLiq Vapor Bypass

Qcc = Qsub - Qleak

Qleak - Qsub + Qcc = 0

• The pressure regulator and vapor bypass valve allow some vapor to flow to the reservoir when needed.

QC

Qsub

Qcc Qsub Qleak

– Re-distribution of LHP internal heat• The required reservoir control heater power Qcc is reduced.• Several variations of this approach.

Introduction to LHP - Ku 2015 TFAWS

– Passive: no heater for bypass valve. A single set point temperature.– Active: bypass valve is controlled by an external heater.

44

Page 45: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

LHP Operating Temperature ControlUse Pressure Regulator and Vapor Bypass

QE

EvaporatorReservoirQCCQcc

Line

quid

Lin

e QPressure Regulator

Vapor Bypass

-Qsub QleakCC, Tcc≡Tset

Condenser

Vapo

r LLiq Vapor Bypass

Qcc = Qsub - Qleak

Qleak - Qsub + Qcc = 0

• The pressure regulator and vapor bypass valve allow some vapor to flow to the reservoir when needed.

QC

Qsub

Qcc Qsub Qleak

– Re-distribution of LHP internal heat• The required reservoir control heater power Qcc is reduced.• Several variations of this approach.

Introduction to LHP - Ku 2015 TFAWS

– Passive: no heater for bypass valve. A single set point temperature.– Active: bypass valve is controlled by an external heater.

45

Page 46: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

LHP Operating TemperatureUse Pressure Regulator and Vapor Bypass

ratu

re

Natural Operating Temperature

Natural Operating TemperatureQE

EvaporatorReservoirQCC

CC

Tem

per

Fixed Operating TemperatureTsetTset

ine

uid

Line QPressure

Regulator

C li Q Q

Heating RequiredCondenser

Vapo

r LLiqu Vapor Bypass

• Advantages

Power InputCooling Req’d

QLow QHigh

QC

Qsub

g– Requires very little CC control heater power.

• Disadvantages– More complex design.

Introduction to LHP - Ku 2015 TFAWS

– Calculation of flow rate through bypass valve is complex. – Additional heater and controller for the pressure regulator

46

Page 47: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

LHP Operating Temperature ControlUse Pressure Regulator and Vapor Bypass

• Passive bypass valve– Yamal 2000 spacecraft, launched in 2003

Payload temperature was controlled within 2K– Payload temperature was controlled within 2K.

• Active bypass valve– TerraSAR satellite– Ground tests demonstrated temperature control within

0.5K for heat load of 5W to 15W and condenser sink temperature between 233K and 308K.

– TerraSAR was launched in 2007. Thermal control system was functioning successfully.

Introduction to LHP - Ku 2015 TFAWS 47

Page 48: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

LHP Operating TemperatureUse TEC

Thermal Strap

TECQE

ure

Natural Operating Temperature

Natural Operating Temperature

Condenser

Vapo

r Lin

e

Liqu

id L

ine

EvaporatorReservoir

CC

Tem

pera

tu

Fixed Operating TemperatureTsetTset

Condenser

Q Qc

Heating Required

• Advantages– Can be used to heat or cool the CC

QSCQc

Power InputCooling Req’d

QLow QHigh

Can be used to heat or cool the CC– Changing the voltage polarity changes the mode of operation– Very efficient

• DisadvantagesM l d i

Introduction to LHP - Ku 2015 TFAWS

– More complex design– Additional mass

48

Page 49: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

Schematic of ST 8 MLHP Use TECs and Coupling Blocks for CC Temperature Control

Heat InThermoelectric Converter

Radiator 1Heat O t

Instrument Simulator 1

Heat InHeat InThermoelectric Converter

Radiator 1Heat O t

Instrument Simulator 1

Evaporator 1CC 1Condenser 1

Radiator 1 Out

Evaporator 1CC 1Condenser 1

Radiator 1 Out

Vapor Line

Liquid Line

Coupling Block Flow Regulator

Vapor Line

Liquid Line

Coupling Block Flow Regulator

CC 2

Liquid Line

Heat In Instrument Simulator 2

CC 2

Liquid Line

Heat InHeat In Instrument Simulator 2

Evaporator 2

CC 2

Thermoelectric Converter Heat

Condenser 2

Radiator 2

Evaporator 2

CC 2

Thermoelectric Converter Heat

Condenser 2

Radiator 2

Condenser 2

Radiator 2

Introduction to LHP - Ku 2015 TFAWS

ConverterOut

ConverterOut

49

Page 50: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

Loop Operating Temperature Control Using TECsPower and Sink Cycle Tests

CETDP T C l T /2 /200CETDP Temperature Control Test 5/25/2005

31025

30

E1 (2)E2 (4)

290

300

RE

(K) 15

20

W)C2 Sink (62)

CC1 (42)CC2 (46)

270

280

TEM

PER

ATU

R

5

10

POW

ER (

W

C1 Sink (59)TEC1 Power TEC2 Power

260-5

0

CC1=303K

E1/E2 = 75W/0W E1/E2 = 0W/75WE1 /E2=75W/0W

CC1/CC2=303K CC2=303K

CC1/CC2= 303K CC1=303K

25011:00 12:00 13:00 14:00 15:00 16:00 17:00 18:00

TIME (HH:MM)

-10

• The loop operating temperature was controlled within ±0.5K by TECs regardless of changes in evaporator power and/or sink temperature and regardless of which CC was

Introduction to LHP - Ku 2015 TFAWS

changes in evaporator power and/or sink temperature, and regardless of which CC was being controlled.

50

Page 51: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

LHP Operating Temperature ControlUse Secondary Evaporator

QCC QEQcc

Primary EvaporatorReservoir

E

1

Qm

m

-Qsub QleakCC, Tcc≡Tset

Secondary Evaporator E

q

E

2

qm

2m

Qcc = Qsub - Qleak

Qleak - Qsub + Qcc = 0

Condenser/Heat Exchanger 21 mm

Qcc Qsub Qleak

• The secondary evaporator forms an LHP within an LHP.• The secondary loop cools the CC by drawing vapor out of the CC.• Degenerates to the regular LHP when the secondary evaporator is not

h t d

Introduction to LHP - Ku 2015 TFAWS 51

heated.

Page 52: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

LHP Operating Temperature ControlUse Secondary Evaporator

atur

e

Natural Operating Temperature

Natural Operating Temperature

QCC QE

CC

Tem

pera

Fixed Operating TemperatureTsetTset

Primary EvaporatorReservoir

E

1

Qm

2m

Heating Required

Secondary Evaporator E

q

E

2

qm

• Advantages– Active cooling of the CC – can quickly reprime the loop

Power InputCooling Req’d

QLow QHigh

Condenser/Heat Exchanger21

mm

– Active cooling of the CC – can quickly reprime the loop– Especially useful for cryogenic LHP for start-up and parasitic heat

control• Disadvantages

Introduction to LHP - Ku 2015 TFAWS

– Needs an additional evaporator and transport lines– Still needs CC control heater

52

Page 53: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

NASA H2-CLHP POWER CYCLING

60.0

70.0Date: 07/20/01 Note: TV chamber shroud was cooled by LN2

6.0

7.0

50.0

K)

5.0

s)

2nd Pump Power

30.0

40.0

Tem

pera

ture

(K

Primary Pump (TC2)

2nd Pump(TC13)

2nd Condenser (TC15)3.0

4.0

Pow

er (W

atts

1st Pump CC(TC11)

10 0

20.0

1 0

2.0

10.0

14:30 15:00 15:30 16:00 16:30 17:00 17:30 18:00 18:30

Cold Finger (TC20)

0.0

1.0

0.0

Primary PumpPower

19:00 19:30 20:00 20:30

Introduction to LHP - Ku 2015 TFAWS 53

Time

Page 54: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

LHP Start-up

• LHP Start-up is a complex phenomenon.

• The primary wick must be wetted prior to start-up.

• The loop start-up behavior depends on initial conditions inside the evaporator.

f f– Vapor grooves on the outer surface of the primary wick• Liquid filled: superheat is required for nucleate boiling• Vapor presence: instant evaporation

– Liquid core on the inner surface of the primary wick• Liquid filled: low heat leak• Vapor presence: high heat leak

• A minimum power is required for start-up under certain conditions.

Introduction to LHP - Ku 2015 TFAWS 54

Page 55: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

Four Start-up Scenarios for LHP

• Vapor grooves– Liquid filled:

superheat is

Tem

pera

ture

Te

TccStart up

Tamb

Tem

pera

ture

Te

Tamb

superheat is required for nucleate boiling

– Vapor presence:

Time

Start-up

Time

TccStart-up

p pinstant evaporation

• Liquid core

(a) Situation 1 (c) Situation 3

– Liquid filled: low heat leak

– Vapor presence: hi h h t l k

Tem

pera

ture

Te

TStart-up

Tamb

Tem

pera

ture

Te

Tcc

Tamb

St thigh heat leakTime

Tcc

Time

Start-up

Introduction to LHP - Ku 2015 TFAWS 55

(b) Situation 2 (d) Situation 4

Page 56: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

Vapor Presence in Vapor Grooves

• Situation 1– Vapor presence in vapor grooves– Core is liquid flooded; low heat leak Te

mpe

ratu

re

Te

TccStart up

Tamb

q– Instant liquid vaporization in grooves– Smooth start-up with no or small

temperature overshoot during start-up

Time

Start-up

transient

• Situation 2

(a) Situation 1

– Vapor presence in vapor grooves– Vapor presence in core; high heat leak– Instant liquid vaporization in grooves

Tem

pera

ture

Te

TccStart-up

Tamb

– Smooth start-up with possible large temperature overshoot during start-up transient

Time

Introduction to LHP - Ku 2015 TFAWS

(b) Situation 2

56

Page 57: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

Worst Case Start-up –Situation 4 Sit ti 4• Situation 4– Vapor grooves are flooded with liquid;

superheat is required for nucleate boiling Te

mpe

ratu

re

Te

Tamb

boiling– Core contains vapor; high heat leak– The CC temperature rises along with the

evaporator temperature

Time

e

TccStart-up

p p– The required superheat may never be

obtained before the maximum allowable temperature is reached.

(d) Situation 4

CC Tra

ture

CCT

ratu

re

Evap

Loop does not start

Tem

per

Evap

Loop starts

Tem

per

Introduction to LHP - Ku 2015 TFAWS

TimeTimeTimeTime

Desired Actual57

Page 58: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

Situation 3 – Choosing Between Two Evils

• Situation 3– Vapor grooves are flooded with liquid;

superheat is required for nucleate boiling Te

mpe

ratu

re

Te

Tamb

boiling– Core is flooded with liquid; low heat

leak– The CC temperature remains constant

Time

TccStart-up

– The CC temperature remains constant or rises slowly while the evaporator temperature is rising

– The required superheat will eventually

(c) Situation 3

ybe reached.

• The current practice for LHP start-up is to flood the entire loop prior to start-up to

t th i k i tt d d t i

CC

E

T

erat

ure

guarantee the wick is wetted, and sustain the burden of potentially high superheat for nucleate boiling at start-up – “the lesser of the two evils”. Time

Evap

Loop starts

TimeT

empe

Introduction to LHP - Ku 2015 TFAWS

TimeTime

Desired and Actual 58

Page 59: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

High and Low Power Start-up

• With high power to the evaporator, liquid in the vapor grooves can be vaporized quickly regardless of the initial two-phase status in the grooves and the evaporator core.– The required superheat, if any, can be achieved in a short time.– Within the short time, the total heat leak is small.

• With low power to the evaporator, start-up could be problematic.– Under situation 4, the required superheat for nucleate boiling

may never be achieved.may never be achieved.– After the loop starts, a steady state may not be established

within the allowable temperature limit at low powers due to a high heat leak from evaporator to CC if the core contains vapor.high heat leak from evaporator to CC if the core contains vapor.

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I di ti f th i ti f l t t

Some Examples of Start-up Tests

• Indication of the inception of loop start-up:– Sudden sharp increase of the vapor line temperature to the

CC saturation temperature– Sudden sharp decrease of the liquid line temperature

• Successful start-upp– The CC temperature approaches a SS– The vapor line temperature approaches a SS (same as or

close to the CC temperature)close to the CC temperature) – The evaporator temperature approaches a SS (slightly

higher than the CC temperature)

• Results of some start-up tests under various conditions follow.

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GLAS LHP Breadboard Start-up(Evaporator core is liquid-filled)

Sit ti 3 t t12/1/97GLAS LHP Start-Up

100 watts, No Controlling, Chiller@0°C, Radiator in Horizontal Position

CompCham(TC2) Evaporator(TC10) VapLine(TC22) LiqLine(TC52) Cart1

Situation 3 start-up

295

300

100

120

power

290

ture

(ºC

) 80

r (W

)

evapcomp cham

280

285

Tem

pera

t

40

60

Pow

er

liq linevap line

270

275

9:15 9:30 9:45 10:00 10:15 10:300

20

vap line

Introduction to LHP - Ku 2015 TFAWS

Time(Hours)

61

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GLAS LHP Breadboard Start-up( Vapor present in evaporator core)

Sit ti 4 t t 100W

GLAS LHP Start-Up100 watts, No Controlling, Chiller@0°C, Radiator in Vertical Position

C Ch (TC2) E t (TC10) V Li (TC22) Li Li (TC52) C t1

Situation 4 start-up: 100W

300

305

100

120

CompCham(TC2) Evaporator(TC10) VapLine(TC22) LiqLine(TC52) Cart1

power

290

295

re (K

)

80

100

W)

evap

comp cham

280

285

Tem

pera

tur

40

60

Pow

er (W

270

275

9 5 9 7 9 9 10 1 10 3 10 5 10 7 10 90

20

vap line

liq line

Introduction to LHP - Ku 2015 TFAWS

9.5 9.7 9.9 10.1 10.3 10.5 10.7 10.9

Time(Hours)

62

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GLAS LHP Breadboard Start-up( Vapor present in evaporator core)

GLAS LHP Testing

Situation 4 start-up: 20W

26Nov1997

320 25

Evaporator CompCham

300

310

15

20Evaporator

Power

CompCham

290 10

LiqLine

270

280

9:00 9:30 10:00 10:30 11:00 11:30 12:00 12:300

5VapLine

Introduction to LHP - Ku 2015 TFAWS

9:00 9:30 10:00 10:30 11:00 11:30 12:00 12:30

Time

63

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Enhancing the Start-up Success

• A small start-up heater is used to achieve the required superheat for nucleate boiling in a localized region to generate the first bubble in vapor grooves.

After vapor is present in grooves liquid evaporation takes place– After vapor is present in grooves, liquid evaporation takes place instead of nucleate boiling, i.e. superheat is no longer required.

• Cool the CC using an active means (e.g. TEC).

Evap

CCT

Loop starts

CC

T

Tem

pera

ture

Evap

CC

Tem

pera

ture

Time

Loop starts

Time

T

Time

Loop starts

Time

Loop startsT

Start-up heater raises the evaporator

Introduction to LHP - Ku 2015 TFAWS

TEC lowers the CC temperatureStart up heater raises the evaporator temperature quickly over a small area

64

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LHP Shutdown• Some instrument operation requires LHP to shutdown for a period of timeSome instrument operation requires LHP to shutdown for a period of time.• LHP can continue to pump fluid if the evaporator temperature is higher

than the CC temperature.• Requirements for LHP shutdownRequirements for LHP shutdown

– No net heat load to evaporator– CC temperature is higher than evaporator temperature

• Heating the CC is the only viable methodHeating the CC is the only viable method

• When the CC temperature is higher than the evaporator temperature, fluid flow stops.p– Loop will not restart as long as there is no net heat load to evaporator. – Loop may restart if the evaporator continues to receive net heat load

and its temperature rises above the CC temperature.• To guarantee that the payload stays above its minimum allowable

temperature, the CC temperature control can be set slightly above that value during loop shutdown.

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Analytical Modeling of LHP

• SINDA/Fluint can be used to model LHP operation.– CAPIL connector and CAPPMP macro to model wick– Phase suction option to model two-phase heat transferPhase suction option to model two phase heat transfer– Tedious and time-consuming to build the detailed LHP model– Run time could be an issue

• Under NASA SBIR and the ST 8 Project, TTH Research Inc. has developed an LHP model specifically for the simulation LHP operationoperation.

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NASA LHP Analytical Model

• Developed by TTH Research, Inc. under NASA SBIR Project in 2002.

• The objective was to develop an analytical model to simulate LHP steady state and transient behaviors– based upon physical laws and verified by test data– efficient and stable solutions– easy to use by thermal analysts (non-experts)– accurate and detailed predictions for LHP researchers

(experts)(experts)– Can be used as a stand-alone model for LHP design, or a

subroutine to general thermal analyzer (e.g. SINDA/Fluint)

• Additional funding for modeling the secondary wick was provided by DOD and the ST8 project in 2005.

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Modeling Approach• Derive governing equations for each component and the overall loop• Derive governing equations for each component and the overall loop

based on mass, momentum and energy balance. – fluid movement based on pressure difference– improved heat leak model based on test datap– two-phase correlations in condenser – database for fluid properties, wick performance characteristics

• Model Assumptions– One dimensional pipe flow– liquid and vapor at one temperature (saturation) inside the reservoir– track liquid level in CC at all times (including gravity effects)

N li ibl t f d bl– Negligible amount of non-condensable gases• Effects of gravity are included in the model.

Gravity

1 g 0-g

Introduction to LHP - Ku 2015 TFAWS

1-g 0-g

Compensation Chamber Fluid Distribution as a function of Gravity

68

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Nodal Map of LHP Analytical ModelFluid-to-Wall G171-G180

510 505 (Pump #5)CC #5WallFluid-to-Wall G171-G180

510 505 (Pump #5)CC #5Wall

Nodes 371 380 (Wall)Fluid-to-Wall G171-G180

510 505 (Pump #5)CC #5Wall

Fluid-to-Wall G161-G170

Fluid-to-Wall G151-G160

Pump #3 Return Line

Pump #4 Return Line

Pump #5 Return Line

508

509

503 (Pump #3)

504 (Pump #4)

CC #3Wall

CC #4WallFluid-to-Wall G161-G170

Fluid-to-Wall G151-G160508

509

503 (Pump #3)

504 (Pump #4)

CC #3Wall

CC #4Wall

Nodes 1151-1160 (Fluid)

Nodes 351 360 (Wall)

Nodes 1161-1170 (Fluid)

Nodes 361 370 (Wall)Nodes 1171-1180 (Fluid)

Node 1308

Node 1309

Node 1310

Node 1303

Node 1304

Node 1305

Fluid-to-Wall G161-G170

Fluid-to-Wall G151-G160508

509

503 (Pump #3)

504 (Pump #4)

CC #3Wall

CC #4Wall

d)l) 0

Fluid-to-Wall G141-G150

Fluid-to-Wall G51-G60

Pump #1 Return Line

Pump #2 Return Line

Pump #3 Return Line

(Fluid in CC #1) (Vapor)

506

507

CC #1Wall 501 (Pump #1)

502 (Pump #2)CC #2WallFluid-to-Wall G141-G150

Fluid-to-Wall G51-G60

(Fluid in CC #1) (Vapor)

506

507

CC #1Wall 501 (Pump #1)

502 (Pump #2)CC #2Wall

20d) )

Nodes 1051-1060 (Fluid)

Nodes 251-260 (Wall)Nodes 1141-1150 (Fluid)

Nodes 341 350 (Wall)

Node 1306

Node 1307

Node 1308

Node 1301

Node 1302

Node 1303

d)d)l) 0

Fluid-to-Wall G141-G150

Fluid-to-Wall G51-G60

(Fluid in CC #1) (Vapor)

506

507

CC #1Wall 501 (Pump #1)

502 (Pump #2)CC #2Wall

Nod

es 1

201-

1220

(Flu

id

Liqu

id L

ine

Nod

es 2

31- 2

50 (W

all

Flui

d-to

-Wal

l G31

-G5

Vapo

r Lin

e

( ) ( p )

Liqu

id L

ine

Flui

d-to

--

( ) ( p )

--W

all G

201-

G22

luid

to

Nod

es 1

031-

1050

(Flu

i d

Nod

es 4

01-4

20 (W

all)

Nod

es 1

201-

1220

(Flu

idN

odes

120

1-12

20 (F

luid

Nod

es 2

31- 2

50 (W

all

Flui

d-to

-Wal

l G31

-G5

( ) ( p )

N

Fluid-to-Wall G1-G20

Fluid-to-Wall G61-G80

Condenser #2

Condenser #1

C d #3

Fluid-to-Wall G21-G30

F

Fluid-to-Wall G1-G20

Fluid-to-Wall G61-G80Fluid-to-Wall G21-G30

F Fl

Nodes 1001-1020 (Fluid)

Nodes 201 220 (Wall)Nodes 1061-1080 (Fluid)

Nodes 261 280 (Wall)

Nodes 1021-1030 (Fluid)

Nodes 221 230 (Wall)

Subcooler

N NNN

Fluid-to-Wall G1-G20

Fluid-to-Wall G61-G80Fluid-to-Wall G21-G30

F

Fluid-to-Wall G1-G20

Fluid-to-Wall G81-G100

Fluid-to-Wall G101-G120

Condenser #3

Condenser #4

Condenser #5

Fluid-to-Wall G81-G100

Fluid-to-Wall G101-G120

( )Nodes 1081-1100 (Fluid)

Nodes 281 300 (Wall)Nodes 1101-1120 (Fluid)

Nodes 301 320 (Wall)Nodes 1121-1140 (Fluid)

Fluid-to-Wall G81-G100

Fluid-to-Wall G101-G120

Introduction to LHP - Ku 2015 TFAWS

Fluid-to-Wall G121-G140Fluid-to-Wall G121-G140( )

Nodes 321 340 (Wall)Fluid-to-Wall G121-G140

69

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LHP Analytical Model Solution Scheme

Two-Step Predictor-Corrector

Thermal Analyzer(e.g. SINDA)

Thermal Analyzer

CALL LHP_INLHPData File

Thermal Analyzer(e.g. SINDA)

CALL LHPNext Time Step

CALL LHP

END

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LHP Analytical Model Input Data Vapor Line

o O.D., wall thickness, length, material Li id Li Liquid Line

o O.D., wall thickness, length, material Condensers

o No. of condensers o Condenser 1 O.D., wall thickness, length, material o Repeat for Condenser 2 Condenser 3 etco Repeat for Condenser 2, Condenser 3, etc.

Subcooler o O.D., wall thickness, length, material

Evaporators o No. of evaporators o Evaporator 1p

Vapor exit line: O.D., wall thickness, length, material Liquid inlet line: O.D., wall thickness, length, material Pump body O.D., length, material Primary wick O.D., I.D., length, material, pore radius,

permeability, porosity, thermal conductivity Bayonet tube: O.D., I.D. Vapor grooves: number of grooves, hydraulic diameter

of each groove Reservoir: O.D., I.D., length, material Adverse elevation

S d i k di bilit Secondary wick: pore radius, permeability, cross sectional area, thermal conductivity, no. of vapor channels, hydraulic diameter of each vapor channel

Start-up initial condition (situation 1, 2, 3 or 4) Superheat at start-up

o Repeat for Evaporator 2 Evaporator 3 etc

Introduction to LHP - Ku 2015 TFAWS

o Repeat for Evaporator 2, Evaporator 3, etc. Gravitational acceleration Working fluid

71

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Model Capabilities

• LHP with up to 5 evaporators and up to 5 condensers• Simulation of steady state or transient behavior• Database for more than 40 working fluidsDatabase for more than 40 working fluids• Database for wick properties based on empirical test data• Default values for input data• Gravity effects included• A FORTRAN subroutine to be used with any thermal analyzer

(e.g. SINDA, TMG)

Introduction to LHP - Ku 2015 TFAWS 72

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Model Limitations

• The analytical model can predict when system pressure drop exceeds capillary limit of primary wick. The model cannot simulate loop behavior thereafter. p

lity Vapor “Blow-Through”

BubblePoint

Prob

abi

M d l d t t k i t t ff t f i ffi i t

Pore Size

• Model does not take into account effects of insufficient liquid in reservoir (undercharged LHP in 1-g)

Introduction to LHP - Ku 2015 TFAWS 73

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Recent LHP Technology Developments

• Miniature LHP– 6.35 mm diameter evaporator

• A Single LHP with Multiple Evaporators and Multiple Condensers

C /• Hybrid CPL/LHP

• Cryogenic LHP– Nitrogen LHP: ~75K-100K– Neon LHP: ~28K-44K– Hydrogen LHP: ~20K-30K– Helium LHP: ~2.7K-4.4K

Introduction to LHP - Ku 2015 TFAWS 74

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CEDTP Miniature Loop Heat Pipes

• Miniature LHPs under NASA CETDP program.– Breadboards built by Swales

d Thand Thermacore

CondenserEvaporator60 cm

Liquid Transport Line

Vapor Transport Line

Transport Lines

CC 9 52mm OD

Evaporator Pump

ReservoirSubcooler

Vapor Line 1.59 mm

6.35 mm OD Evaporator

CC 9.52mm OD

TEC

Counter-flow Condenser

Liquid line 1 59

ODTEC Saddle

Introduction to LHP - Ku 2015 TFAWS

Liquid line 1.59 mm OD

75

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Mini LHP for CCQ Flight Experiment

• Made by RussiansCylindrical Evaporator inside block for heatersCompensation

Chamber • Flown for CCQ Flight Experiment (2012)

Chamber

Flat evaporator with integral compensation

chamber

Introduction to LHP - Ku 2015 TFAWS 76

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ST8 Thermal Loop - LHP Installed on Test Frame

Evap2

Li id li

Vapor lineVapor lineEvap2

Li id li

Vapor lineVapor line

CC 2Liquid line

Evap2CC 2

Liquid lineCC 2

Liquid lineEvap2

CC 2Liquid line

Evap1 CC 1

C d 2

Evap1

CC 1Evap1 CC 1

C d 2

Evap1

CC 1

Condenser 1Condenser 2

Condenser 1Condenser 2

Condenser/Radiator 2 Condenser/Radiator 1Condenser/Radiator 2 Condenser/Radiator 1

• A single LHP with two evaporators and two condensers• Miniature LHP

Introduction to LHP - Ku 2015 TFAWS77

• Miniature LHP• TECs for reservoir temperature control

Page 78: Introduction to Loop Heat Pipes - NASA AURA, 5 LHPs Launched July 2004 Introduction to LHP - Ku 2015 TFAWS 8 ICESat, 2 LHPs Launched Jan 2003 SWIFT, 2 LHPs Launched Nov 2004 GOES N-Q,

Cryogenic Loop Heat Pipe (CLHP)

INQRQ

INT

Primary EvaporatorReservoir

E

1Q

mOUTx

Line L

ine

asiti

c H

eat

SecondaryEvaporator

1

INq2m

S d C d

Vap

or L

d L

ine

econ

dary

Flu

id

Par

a

The Innovation

2m

21 mm Primary Condenser

Secondary Condenser

Liqu

id S

Pressure Reduction“Hot” Reservoir

• Nitrogen CLHP• Hydrogen CLHP

Introduction to LHP - Ku 2015 TFAWS 78

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CLHP for Large Area Cryocooling

• Delivered by TTH Research in 2007

X

X

XB2B5 B7B1

A1

Evaporator Plate

• Manufactured by Thermacore, Inc.

XX

X

XX

B6

A2

B2B5 B7B1

B3

XB8

Reservoir

Condenser Plate

XA5

XA6

X

X

A3

A4

A8 on 2nd Shroud Bottom

Capillary Pump

XA7B4 on 2nd Shroud Top

• CLHP– all stainless steel construction

• Evaporator Plate– copper 10” 48 in2

– capillary pump: 1/4”OD x 1.5”L– wick: 1.2m x 45% porosity– reservoir: 1/4”OD x 2.5”L

• Condenser Plate– copper 3” x 5.5” x 1”

Introduction to LHP - Ku 2015 TFAWS

– transport line: 1/16”OD x 63”L • Hot reservoir– 1000 ml (not shown)

79

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Other Advanced Topics Not Covered in This Course

• Temperature Oscillations in LHPs

T t H t i• Temperature Hysteresis

• Effect of Secondary Wick on LHP Transient Operation

• Start-up and Re-start due to Reservoir Cold Shock

• Multiple LHPs Serving a Single Components (Swift ABT , GOES-R ABI, and GOES-R GLM)

• Gravity Effects

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LHP Summary (1 of 3)

K t hi h h t t t f LHP• Key to high heat transport of LHP– Metal wicks with very fine porous wick– High thermal conductivity affects operating temperature

K t b t LHP ti• Key to robust LHP operation– Integral evaporator and CC design– Secondary wick connecting CC to evaporator: vapor tolerant

K t d t di LHP ti• Key to understanding LHP operation– CC saturation temperature governs the loop operating temperature– CC is plumbed in line with flow circulation

CC t t it lf ff t d b ti diti– CC temperature itself affected by operating conditions – Thermodynamic constraints: P is linked to T – CC volume and liquid inventory

K d i i CC i• Key to determining CC saturation temperature– Net heat gain must be balanced by subcooling of returning liquid– Ambient temperature affects liquid subcooling

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LHP Summary (2 of 3)• Heat leak from evaporator to CC affectsHeat leak from evaporator to CC affects

– Loop natural operating temperature– Overall system thermal conductance– Temperature hysteresisce– Temperature hysteresisce

• Heat leak from evaporator to CC is affected by– Wick thermal conductivity

Heat load to the evaporator– Heat load to the evaporator– Two-phase status inside the evaporator core

• Liquid subcooling is affected byHeat load to the evaporator– Heat load to the evaporator

– Temperature difference between sink and ambient– Parasitic heat gain/loss along the liquid line

• CC sizing and liquid inventory• CC sizing and liquid inventory– Determined concurrently– Must satisfy cold start-up and hot operating conditions

Loop must not become liquid filled at maximum non operating

Introduction to LHP - Ku 2015 TFAWS

– Loop must not become liquid-filled at maximum non-operating temperature.

82

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LHP Summary3 of 3

• The thermodynamic constraint (P versus T) affects – Normal operation – Start-upStart up– Operation with presence of body force and/or NCGs– Operation of an LHP with multiple evaporators– Operation of multiple LHPsOperation of multiple LHPs

• Operating temperature range• Never operate LHP near the freezing point except for rare• Never operate LHP near the freezing point except for rare

extremely cold start-up transients• Never operate LHP near the critical point

Introduction to LHP - Ku 2015 TFAWS 83

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Questions?Questions?

Introduction to LHP - Ku 2015 TFAWS 84


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