Satellite Thermal Control Engineering
Transcript of Satellite Thermal Control Engineering
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SME04, 25jun04, [email protected] 1 of 66ESTEC
Thermal & Structure Division
Satellite Thermal Control Engineering
[email protected] Space Agency, Estec, Thermal and Structure DivisionKeplerlaan 1, PO Box 299, 2200AG Noordwijk, The Netherlands
Tel +31 715654554, Fax +31 715656142
prepared for “SME 2004"
ISS
ENVISATERS
L1
HIPPARCOS
ECS
OLYMPUS
ARTEMIS
SPACELAB
ISO
ULYSSES
HUYGENS
SOHO
GIOTTO
CASSINI
MSG
ARIANE
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SME04, 25jun04, [email protected] 2 of 66ESTEC
Thermal & Structure Division
Satellite Thermal Control Engineering
1. heat transfer basics– conduction
– radiation
– importance of thermo-optical properties
2. satellite energy balance– from ground to space
– simple satellite thermal behaviour
3. role– why thermal control required?
4. design– what is thermal design?
– which types of S/C design exist?
5. means– what to control the
flux/temperatures
What you will learn?
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SME04, 25jun04, [email protected] 3 of 66ESTEC
Thermal & Structure Division
ROSETTA* FM in LSS, dec01
*without Solar Panels
1. Heat Transfer Basics
Thermal Control Engineering1. heat transfer basics
2. satellite energy balance
3. role
4. design
5. means
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SME04, 25jun04, [email protected] 4 of 66ESTEC
Thermal & Structure Division
ROSETTA* FM in LSS, dec01
*without Solar Panels
1.1 Satellite Heat Transfer Modes
1. Heat Transfer Basics1.1 satellite heat transfer modes
1.2 conduction
1.3 radiation
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SME04, 25jun04, [email protected] 5 of 66ESTEC
Thermal & Structure Division
1.1 Satellite Heat Transfer Modes
• Conduction– between any body– eventually by contact through an interface
• Radiation– main mode of heat transfer in vacuum/space
• Convection– manned tended satellites (ISS, shuttle, launchers, ascent…)
• Ablation– combination of 3 and chemical reaction (re-entry vehicles)
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SME04, 25jun04, [email protected] 6 of 66ESTEC
Thermal & Structure Division
ROSETTA* FM in LSS, dec01
*without Solar Panels
1.2 Conduction
1. Heat Transfer Basics1.1 satellite heat transfer modes
1.2 conduction
1.3 radiation
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SME04, 25jun04, [email protected] 7 of 66ESTEC
Thermal & Structure Division
1.2 Conduction
• Definition– propagation of energy from particle to particle– in solid, liquid or gaseous continuous matter, homogeneous or not– without matter displacement
• Fourier’s Law
– is the heat flow rate vector (W/m2) – is the material thermal conductivity (W/m2.K)– one-dimensional conduction
Tkq ∇−=rr
qr
k
qr
T(x,y,z)nr
( )ch TTlAk
Q −=
T(x)Th Tc
A
l
k
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SME04, 25jun04, [email protected] 8 of 66ESTEC
Thermal & Structure Division
1.2 Conduction - Data
1.E-04
1.E-03
1.E-02
1.E-01
1.E+00
1.E+01
1.E+02
1.E+03
1 10 100 1000
Temperature (K)
Thermal Conductivityk
(W/m
.K)
Copper
Aluminium
AA5083-T0
304 ss
G-10 // to warp
Ti
Epoxy
PE //
Cu-Ni (70-30)
Brass Cu-Zn
Mylar PET amorphous
(90-10)
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SME04, 25jun04, [email protected] 9 of 66ESTEC
Thermal & Structure Division
ROSETTA* FM in LSS, dec01
*without Solar Panels
1.3 Radiation
1. Heat Transfer Basics1.1 satellite heat transfer modes
1.2 conduction
1.3 radiation
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SME04, 25jun04, [email protected] 10 of 66ESTEC
Thermal & Structure Division
1.3 Radiation
• Characteristics– propagation of electro-magnetic energy in straight line– between surfaces separated by
• absorbing, scattering media• or in vacuum
– hence without matter displacement– reflected, absorbed or transmitted on surrounding bodies
• Source– thermal agitation of particles
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SME04, 25jun04, [email protected] 11 of 66ESTEC
Thermal & Structure Division
1.3 Radiation - Black Body
• Black Body– is real or fictitious surface– that absorbs all incident radiant energy i.e.
• from every direction• at every wavelengths
– isotropic emitter• radiated energy depends only on temperature
• Black Body Emitted Energyhemispherical spectral hemispherical total
emissive power emissive power
(W/m2.µm) (W/m2)
−
=
1
2
5
2
,
TkchT
Be
chE
λ
λ
λ
π4
0,, TdEE TTbb σλλ == ∫
∞
Planck’s LawStefan-Boltzmann’s Law
( ) 1, == αλθα
( ) 1, == ελθε
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SME04, 25jun04, [email protected] 12 of 66ESTEC
Thermal & Structure Division
1.3 Radiation – Black BodyPlanck and Stefan-Boltzmann Laws
0.0
0.2
0.4
0.6
0.8
1.0
0.1 1.0 10.0 100.0λ, Wavelength (µm)
E λ,Τ, H
emis
pher
ical
Spe
ctra
lEm
issi
ve P
ower
(1014
W/m
2 .µm
)
0.00
0.25
0.50
0.75
1.00
1.25
1.50
5776 K
255 K
SUN EARTH
0.5 µm12 µm
Area = σ TE4
Eλ,Τ , H
emispherical Spectral
Emissive Power (10
7 W/m
2. µm)
Area = σ TS4
Planck and Stefan-Boltzmann Laws
0.0
0.2
0.4
0.6
0.8
1.0
0.1 1.0 10.0 100.0λ, Wavelength (µm)
E λ,Τ, H
emis
pher
ical
Spe
ctra
lEm
issi
ve P
ower
(1014
W/m
2 .µm
)
0.00
0.25
0.50
0.75
1.00
1.25
1.50
5776 K
255 K
SUN EARTH
0.5 µm12 µm
Area = σ TE4
Eλ,Τ , H
emispherical Spectral
Emissive Power (10
7 W/m
2. µm)
Area = σ TS4
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SME04, 25jun04, [email protected] 13 of 66ESTEC
Thermal & Structure Division
1.3 Radiation - Real Body
• can absorb, reflect or transmit radiation energy
- all parameters are wavelength andangular dependent
- general case: semi-transparent
- opaque
hence
( ) ( ) ( ) 1=++ λτλρλα
Φλ incident
ρs Φλspecularlyreflected
ρd Φλ diffuselyreflected
α Φλ absorbed
τ Φλ transmitted ( ) 0=λτ
( ) ( ) 1=+ λρλα
ds ρρρ +=
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SME04, 25jun04, [email protected] 14 of 66ESTEC
Thermal & Structure Division
• Surface Emissivity– ratio of surface radiated energy to that of a black body at the same T– always <1 for a real surface
for a black body
– depends on direction θ and wavelength λ of emitted energy– therefore can be
• directional (d) or hemispherical (h)• spectral (s) or total (t)• averaged over all directions, wavelengths or both
1.3 Radiation - Real Body
( ) 1,
0,
0,,
<=
∫
∫∞
∞
λ
λαλθε
λ
λλ
dE
dE
T
TT
( ) 1, == ελθε
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SME04, 25jun04, [email protected] 15 of 66ESTEC
Thermal & Structure Division
• Surface Absorptivity– ratio of surface absorbed energy to incident energy– always <1 for a real surface
for a black body
– depends on incident energy direction θ and wavelength λ– therefore can be
• directional (d) or hemispherical (h)• spectral (s) or total (t)• averaged over all directions, wavelengths or both
1.3 Radiation - Real Body
( ) 1,
0,
0,,
<=
∫
∫∞
∞
λ
λαλθα
λ
λλ
dE
dE
T
TT
( ) 1, == αλθα
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SME04, 25jun04, [email protected] 16 of 66ESTEC
Thermal & Structure Division
• Absorptivity vs Emissivity– for a given direction θ and at any wavelength λ
– in general hemispherical total values are different
because
– α and ε have a strong wavelength dependence
– source temperature of incident radiation (Sun at 5776 K) differentthan surface temperature (satellite –250 -> 300°C)
1.3 Radiation - Real Body
( ) ( ) λθλθελθα ∀∀= ,,,2nd Kirchoff’s Law
εα ≠
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SME04, 25jun04, [email protected] 17 of 66ESTEC
Thermal & Structure Division
• Solar Absorptivity αS and Hemispherical Emissivity εH
αS is the solar absorptivity ⇒ refers to UV wavelengthsαS = εS integrated over 0.2-2.8 µm i.e. 95% solar spectrum
εH is the hemispherical emissivity ⇒ refers to IR wavelengthsαH = εH integrated over 5-50 µm i.e. body at –250/300°C
but αS ≠ εH because the spectra are different
1.3 Radiation - Real Body
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SME04, 25jun04, [email protected] 18 of 66ESTEC
Thermal & Structure Division
1.3 Radiation - Data
• Spectral Reflectance ρ– Zinc Oxide Potassium
Silicate Coating
• Black Body Emittance – integration over solar
(5776K) wavelengths• αs=0.20
– integration overinfraredblack body (300K) wavelengths
• εh=0.87
MAP PSG120-FD Reflectance
0.0
0.3
0.5
0.8
1.0
1.3
1.5
0.1 1.0 10.0 100.0
λ, Wavelength (µm)
E λ,Τ, H
emis
pher
ical
Spe
ctra
lEm
issi
ve P
ower
(1014
or
107 W
/m2 .µ
m)
0.00
0.25
0.50
0.75
1.005776 K255 KReflectance
0.5 µm
ρ, Spectral Reflectance (-)
12 µm
MAP PSG120-FD Reflectance
0.0
0.3
0.5
0.8
1.0
1.3
1.5
0.1 1.0 10.0 100.0
λ, Wavelength (µm)
E λ,Τ, H
emis
pher
ical
Spe
ctra
lEm
issi
ve P
ower
(1014
or
107 W
/m2 .µ
m)
0.00
0.25
0.50
0.75
1.005776 K255 KReflectance
0.5 µm
ρ, Spectral Reflectance (-)
12 µm
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SME04, 25jun04, [email protected] 19 of 66ESTEC
Thermal & Structure Division
1.3 Radiation - Data
• Typical Values
Finish αS εH αS/εH
VD Au 0.23 0.03 9.20VDA 0.15 0.05 3.00black paint 0.94 0.81 1.16white paint 0.20 0.88 0.23SSM (Ag 2 mils) 0.10 0.60 0.17OSR 0.09 0.82 0.11
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SME04, 25jun04, [email protected] 20 of 66ESTEC
Thermal & Structure Division
1.3 Radiation - Black Body
• Radiated Energy between Black Bodies
with Fij, the view factorbetween surface i and surface j
or
when
( )44jiijiij TTFAQ −= σ Ai
AjTi
Tj
Qij
dAi
dAj
( )44jiiij TTAQ −= σ
1=ijF
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SME04, 25jun04, [email protected] 21 of 66ESTEC
Thermal & Structure Division
ROSETTA* FM in LSS, dec01
*without Solar Panels
2. Satellite Energy Balance
Thermal Control Engineering1. heat transfer basics
2. satellite energy balance
3. role
4. design
5. means
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SME04, 25jun04, [email protected] 22 of 66ESTEC
Thermal & Structure Division
2. Satellite Energy Balance
WHAT HAPPENS from
GROUNDto
SPACE ?
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SME04, 25jun04, [email protected] 23 of 66ESTEC
Thermal & Structure Division
• Ultra-high Vacuum, 10-14 bar < p < 10-17 bar => no convection– temperature levels
• Deep Space, @ 2.7 K– imbalance, temperature levels and gradients
• Solar Eclipse– SSO SPOT, ENVISAT 32 mn– GEO MSG 72 mn– HEO CLUSTER 5 h max
2. Satellite Energy Balance - Thermal Environment
0°52’
PENUMBRA
PENUMBRA
UMBRA
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SME04, 25jun04, [email protected] 24 of 66ESTEC
Thermal & Structure Division
• intense Solar Flux, SC=1367 W/m2 @ 1 AU– imbalance, temperature levels and gradients
2. Satellite Energy Balance - Thermal Environment
2S
S dSC
=Φ
Solar Intensity vs Sun Distance
1
10
100
1000
10000
100000
1000000
0.1 1 10Sun Distance (AU)
Inte
nsit
y (W
/m2 )
0.0
0.1
1.0
10.0
100.0
Solar Intensity (SC)
Earth
Mercury
Saturn
Mars
Jupiter
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SME04, 25jun04, [email protected] 25 of 66ESTEC
Thermal & Structure Division
2. Satellite Energy Balance - Thermal Environment
• Albedo Flux – reflected by Sun illuminated side of Planet– albedo = ratio of solar reflected energy to
local solar flux– Earth albedo
aE = 0.33 ± 0.13 equivalent to 410 W/m2
– aE varies with landscape clouds 0.4-0.8forest 0.05-0.10 ocean 0.05
• Planet Flux – infrared energy radiated by the Planet– Earth=blackbody @255 K (-18 °C)
equivalent to 240 W/m2
incident
2ERSCa πSC
2)1( ERSCa π−
reflected
absorbed
24 4 EE RT πσemitted
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SME04, 25jun04, [email protected] 26 of 66ESTEC
Thermal & Structure Division
2. Satellite Energy BalanceEquilibrium Temperature of a Spherefrom Ground to Space
0.1
1.0
10.0
100.0
1000.0
10000.0
100000.0
-120-80 -40 0 40 80 120 160 200
240
Temperature (degC)
Alt
itud
e (k
m)
BlackWhite
Gold
Air
Equilibrium Temperature of a Spherefrom Ground to Space
0.1
1.0
10.0
100.0
1000.0
10000.0
100000.0
-120-80 -40 0 40 80 120 160 200
240
Temperature (degC)
Alt
itud
e (k
m)
BlackWhite
Gold
Air
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SME04, 25jun04, [email protected] 27 of 66ESTEC
Thermal & Structure Division
2. Satellite Energy Balance - Black Sphere
• Assumptions– satellite=black sphere hence α=ε=1– infinitely conductive, deep space at 0 K– low orbit around Earth
• in Sun– no Planet, no albedo
( ) ( ) 422 4 Trqr S σππ =
4
4T
qS σ=
CT o5=
r
α=ε=1
TqS
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SME04, 25jun04, [email protected] 28 of 66ESTEC
Thermal & Structure Division
2. Satellite Energy Balance - Black Sphere
• in Sun with Earth– no albedo
( ) ( ) ( ) 42422 44 TrTrFqr ES σπσππ =+
44
24T
Tq ES σσ
=+
CT o27=
r
α=ε=1
TqS
Earth
ET
F=1/2
CT o22=∆
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SME04, 25jun04, [email protected] 29 of 66ESTEC
Thermal & Structure Division
2. Satellite Energy Balance - Black Sphere
• in Sun with Earth and Albedo
( ) ( ) ( ) ( ) 422422 444 TrqarFTrFqr SES σππσππ =++
44
2241
TT
qa E
S σσ
=+
+
CT o56=
Earth
ETr
α=ε=1
TqS
F=1/2
albedo=a qSqS
CT o29=∆
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SME04, 25jun04, [email protected] 30 of 66ESTEC
Thermal & Structure Division
2. Satellite Energy Balance - Real Body
sq
sq
iisi, aAFsqsolar absorbed
albedo absorbed
)T(TsFA eQ 4p
4ipi,iip −=
radiated to planet
)T(TsFA eQ 4space
4ispacei,iir −=
radiated to deep space
iiai, aAFasq
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SME04, 25jun04, [email protected] 31 of 66ESTEC
Thermal & Structure Division
• Real Body in Sun– assumes that body in infinitely conductive, no albedo, no planet flux– assumes that sink temperature is 0 K (not far from deep space)
T is independent of area Adepends only of α/ε
where FS is the projected area with qs = 1367 W/m2
2. Satellite Energy Balance - Real Body
4TAqA ss σεα =
AA
F ss =
4
σεα s
sq
FT = KFT s 39444
εα=
AAsqs
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SME04, 25jun04, [email protected] 32 of 66ESTEC
Thermal & Structure Division
flat plate cylinder sphere
n
Sθ
l
w
hn
S
θr
r
(W/m2) (-) blac
kbo
dy
whi
te p
aint
PS
G12
0-F
D
blac
k pa
int
Ele
ctro
dag
501
VD
Au
VD
A
sand
-bla
sted
Al
blac
kC
FR
P
S α 1.00 0.20 0.94 0.23 0.15 0.20 0.901367.0 ε 1.00 0.88 0.81 0.025 0.05 0.20 0.80
α/ε 1.00 0.23 1.16 9.20 3.00 1.00 1.13
Surface FS Ap / A
1-s plate 1 1.00 121 -1 136 413 245 121 1332-s plate 1/2 0.50 58 -44 71 304 163 58 68cylinder 1/π 0.32 23 -69 34 242 116 23 32sphere 1/4 0.25 5 -81 16 212 94 5 14
cube 1/6 0.17 -21 -99 -12 165 58 -21 -14
Steady-State Temperature (degC)
for θ=0, TS = 0 K and qs = 1367 W/m2
PLAY withα/ε
RATIO
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SME04, 25jun04, [email protected] 33 of 66ESTEC
Thermal & Structure Division
2. Satellite Energy Balance - Real Body
AAsqs
qa = a qs qp
TsBs
( ) QqAFqAFqAFTTBA ppaassSS +++=− εαασε 44
• Steady-state: General Case– assumes that body in infinitely conductive – solar, albedo and planet fluxes– view factor to sink temperature at Ts≠0 K
Fs, Fa, Fp solar, albedo, planet factors (-)qs, qa, qp solar, albedo, planet fluxes (W/m2)
a albedo factor (-) α solar absorbtivity (-)Ts sink temperature (K) ε infrared emissivity (-)BS Gebhart factor to sink (-) A radiative area (m2)Q power dissipation (W)
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SME04, 25jun04, [email protected] 34 of 66ESTEC
Thermal & Structure Division
when sink Ts surrounds (BS=1) body at T and only solar flux qs
2. Satellite Energy Balance - Real Body
AAsqs
qa = a qs qp
Ts
Bs
( )4
44
σεσεα
SSp
S
ps
S
as
BAQ
TTB
FqB
FaFT +++
+=
4 4S
ss T
qFT +=
σεα
solar infrared dissipation
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SME04, 25jun04, [email protected] 35 of 66ESTEC
Thermal & Structure Division
2. Satellite Energy Balance - Examples
•s
ULYSSES(1989)
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SME04, 25jun04, [email protected] 36 of 66ESTEC
Thermal & Structure Division
2. Satellite Energy Balance - Examples
ISO(1995)
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SME04, 25jun04, [email protected] 37 of 66ESTEC
Thermal & Structure Division
2. Satellite Energy Balance - Examples
ARTEMIS(2001)
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SME04, 25jun04, [email protected] 38 of 66ESTEC
Thermal & Structure Division
ROSETTA* FM in LSS, dec01
*without Solar Panels
3. Role
Thermal Control Engineering1. heat transfer basics
2. satellite energy balance
3. role
4. design
5. means
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SME04, 25jun04, [email protected] 39 of 66ESTEC
Thermal & Structure Division
3. Role
• maintain within Specified Ranges– temperatures– temperature gradients (K/length)– temperature stability (K/time)– radiative/conductive
heat flow (W)
On Board Data Compression Unit (ALS)
SPOT 5 Solid State Recorder (ALS)
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SME04, 25jun04, [email protected] 40 of 66ESTEC
Thermal & Structure Division
3. Role
• of What?– electronic units– instrument e.g. optical bench– S/C structure– interface between modules
Visual Monitoring Camera (AST)
SOHO, STM
SVM
15 Instruments
PLM
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SME04, 25jun04, [email protected] 41 of 66ESTEC
Thermal & Structure Division
3. Role - Typical Requirement
• Narrow Temperature Ranges– electronics equipment
• classical equipment [ -10, +40] °C• battery [ 0, +20] °C• propulsion system [ +10, +50] °C
• limited Temperature Gradients– ∆T < 5°C across optical instrument (1.5 m)– ∆T/∆x < 2°C/m for structural element– ∆T < 5°C between MMH and NTO tanks
• Stable Temperatures– ∆T/∆t < 5 K/h for typical electronic unit– ∆T/∆t < 0.1 K/mn for CCD camera– ∆T/∆t < 100 µK/mn for cryogenic telescope
• Why is it so important?– low temperatures for reliability of components– narrow temperature ranges for sensitivity of detectors, units– small temperature gradients for pointing of instruments, S/C
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SME04, 25jun04, [email protected] 42 of 66ESTEC
Thermal & Structure Division
ROSETTA* FM in LSS, dec01
*without Solar Panels
4. Design
Thermal Control Engineering1. heat transfer basics
2. satellite energy balance
3. role
4. design
5. means
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SME04, 25jun04, [email protected] 43 of 66ESTEC
Thermal & Structure Division
external loads
internal loads
fluid flow(not visualised)
radiated* fluxconducted* flux
4. Designstored energy
* convective
Node iTi mCi α i ε i
Node jTj
Node kTk
conduction*
C ij(Ti-Tj)
radiation
Rijσ(Ti4-Tj
4)
radiation
Rikσ(Tk4-Ti
4)
SpaceNode s
Ts
conduction*
C ik(Tk-Ti)
Planet IRAlbedo UV
radiationRisσ(Ti 4-Ts 4)
Solar UV
*incl. to space *excl. to planet
*/convective
ei
ii
jijij
jijij
jijij QQ+)T(T F+)T(Ts R+)T(T C +−−− ∑∑∑ 44( ) =i dt
dTmC i
P
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SME04, 25jun04, [email protected] 44 of 66ESTEC
Thermal & Structure Division
4. Design
• through Heating– absorb from external sources (solar, albedo, planet IR)
• selective coatings– use the internal sources
• electronic dissipations, MLI insulation efficiency– dissipate heat internally
• heater• RTG, RHU
Balance HEAT FLOWSBalance HEAT FLOWSto fulfil
REQUIREMENTSREQUIREMENTSresults in
TEMPERATURESTEMPERATURES
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SME04, 25jun04, [email protected] 45 of 66ESTEC
Thermal & Structure Division
4. Design
– transfer heat from hot area• conduction, radiation• latent heat of evaporation/condensation
• or through Cooling– reject to deep space (3 K)
• with low α/ε radiative coatings on radiators– transfer heat to cold area
• by conduction,• radiation• through condensation/boiling in fluid loops or heat pipes
– through cryogenic techniques• cryostats• coolers (Peltier, Joule-Thomson…)
– ablation
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SME04, 25jun04, [email protected] 46 of 66ESTEC
Thermal & Structure Division
4. Design – Radiative Concept
• Principle– when internal power dissipation small w.r.t.
external absorbed energy – balance between
• absorbed incident radiant energy (solar…) • emitted radiant energy (σT4)
• Characteristics– no insulation– average temperature driven by
• external fluxes– local temperature hot spots still possible
• Application: PROBA1
PROBA1 FM
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SME04, 25jun04, [email protected] 47 of 66ESTEC
Thermal & Structure Division
4. Design – Insulated Concept
• Principle– when heat source irradiates few sides
• Sun, planet IR (Mercury, Mars, Moon)– balance between
• internally dissipated power (P)• emitted radiant energy (σT4)
• Characteristics– insulation of Sun illuminated sides (MLI)– shadow sides
• with high IR emissivity• radiate to deep space => RADIATORS
– preferred attitude for radiators– average temperature driven by
• internal power dissipation– local temperature hot spots still possible
HYPPARCOS FM, 1990
XMM FM1999
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SME04, 25jun04, [email protected] 48 of 66ESTEC
Thermal & Structure Division
4. Design – Insulated Concept
• Advantages w.r.t. Radiative Concept– less sensitive to
• eclipses• external loads changes
– temperatures are more uniform– little ageing of unirradiated coatings
We are betweenthose
2 CONCEPTS
ASTRA-1K FM Antenna Deployment
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SME04, 25jun04, [email protected] 49 of 66ESTEC
Thermal & Structure Division
ROSETTA* FM in LSS, dec01
*without Solar Panels
5. Means
Thermal Control Engineering1. heat transfer basics
2. satellite energy balance
3. role
4. design
5. means
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SME04, 25jun04, [email protected] 50 of 66ESTEC
Thermal & Structure Division
5. Means - Limitations
• Cooling Limitations– radiator 100 mW at 100 K for 0 W dissipation– cryo-coolers 1 W at 50 K for 100 W dissipation– liquid He few mW at 4 K for 1 ton/2 years
• Heat Transport Limitation/Performance– conduction (pure Al tube k=200 W/m.K)1.5 W @20°C l=1.00 m Ø=2 cm ∆T= 25 K m= 0.8 kg11 kW@20°C l=0.70 m Ø=4.04 m ∆T= 3 K m= 24 t
– heat pipe (Al tube)11 kW @20°C l=0.70 m Ø=2.5 cm ∆T= 3 K m= 2 kg– radiation (from a black surface ε=1)11 kW @20°C A= 88 m2 ∆T= 25 K11 kW @20°C A= 27 m2 ∆T= 290 K
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SME04, 25jun04, [email protected] 51 of 66ESTEC
Thermal & Structure Division
5. Means
HEATERS
- thermostat control - electronic control- ground control
HEAT PIPES - FLOOPS
- fixed/variable conductance- loop heat pipe- monophasic/diphasic fluid
LOUVRES
COOLERS- mechanical- electrical
CONDUCTION
- structural material
- doubler, filler, adhesive
- washer, strap, bolt, tyrap,stand-off
- foam
PASSIVEACTIVE
ENERGYTRANSFER
ENERGYTRANSFER
TlA
k ∆4TA
As
σε
φα
PASSIVEACTIVE
RADIATION- coating- absorber- MLI blanket- radiator
ENERGYCONTRIBUTION
ENERGYCONTRIBUTION
LATENT HEAT-ABLATION- TPS- PCM
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SME04, 25jun04, [email protected] 52 of 66ESTEC
Thermal & Structure Division
5. Means
• Passive Systems Pros/Cons– no mechanical moving parts or moving fluids, no power consumption
• simple to design/implement/test• low mass and cost• highly reliable
– BUT low heat transport capability• except heat pipes
• Active Systems Pros/Cons– mechanical moving parts or moving fluids or electrical power required
• complex design• generate constraints on S/C design and test configurations• high mass and cost• less reliable than PTC means
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SME04, 25jun04, [email protected] 53 of 66ESTEC
Thermal & Structure Division
5. Means - PTC – Radiation, Coatings
• controls Heat absorbed by External S/C Surfaces– with α, solar absorptivity
• controls Heat radiatedto Space– with ε, IR emissivity
Coated Sphere Equilibrium Temperature in Sun
α/ε=10500 K
α/ε=2337 K
α/ε=1.5314 K
α/ε=1284 K
α/ε=0.75264 K
α/ε=0.5238 K
α/ε=0.25200 K
ε
α
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SME04, 25jun04, [email protected] 54 of 66ESTEC
Thermal & Structure Division
5. Means - PTC - Radiation, MLI Blankets
• Purpose– insulating material– acts as a radiation barrier– decreases heat flow inside S/C
• Sun, albedo, IR planet• ascent aerothermal after fairing jettison• ME/ABM firing
– decreases heat losses from S/C• IR energy
• Principle– stack of n layers with low emissivity ε– connected only by radiation with limited
contact areas– equivalent to reduce the emissivity by n
ε/n
Thot
Tcold
Thot
Tcold
εεεε
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SME04, 25jun04, [email protected] 55 of 66ESTEC
Thermal & Structure Division
5. Means - PTC - Radiation, MLI Blankets
• Standard MLI– stack of thin polymer foils
• Kapton®, Mylar® (5-25 foils)– separated (avoid contact) by
• spacer/mesh (Dacron®/Trevira®)• embossed, crinkled• perforated or not
– 1 x bka/VDA-net unperf. 1 mil space exposed side3-23 x VDA/my/VDA-net perf. 0.25 mil internal layers1 x VDA/my or ka/VDA perf. 1 mil innermost layer
– attachment• stand-offs + clip washers• sewed/glued velcro• dacron yarn
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SME04, 25jun04, [email protected] 56 of 66ESTEC
Thermal & Structure Division
5. Means - PTC - Radiation, Radiators
satellite
Qlosses
Qelectric
Qspace
insulation
• Purpose– cool detectors, optical components, mirrors– improve the performances of
• Scientific P/L (all wavelength ranges)• Earth observation (mainly IR)
• Principle– direct coupling to deep space @2.73 K
– heat lift decreases in T4 6 W/m2 @100K
losseselectricspace QQQ +=
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SME04, 25jun04, [email protected] 57 of 66ESTEC
Thermal & Structure Division
5. Means - PTC - Radiation, Radiators
INTEGRAL STM
radiators
MLI
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SME04, 25jun04, [email protected] 58 of 66ESTEC
Thermal & Structure Division
5. Means - PTC – Conduction, Increase
doubler
honeycombfacesheets
• Thermal Doublers– spread heat dissipation under unit– 1 mm thick Al alloy sheet
• Straps/Braid (detector to radiator)– Cu, Al alloy wrapped in MLI/SLI– short < 10 cm
• Contact Area
• Structural Material Selection– Al alloy 120-170 W/m.K– Ti alloy 7-15 W/m.K– steel 10-40 W/m.K
radiator
unit
S/C structure
strap
S/C wall
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SME04, 25jun04, [email protected] 59 of 66ESTEC
Thermal & Structure Division
5. Means - PTC – Conduction, Increase
filler
unit
honeycomb
• Interface Fillers– better unit to S/C conductance– graphite (Sigraflex®)
• laminated graphite sheet• electrical conductor• thickness 0.25 mm
– silicone elastomer (Cho-therm® 1671)• silicone binder, filled with boron nitride
particles, reinforced with fibreglass cloth
• electrical isolator
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SME04, 25jun04, [email protected] 60 of 66ESTEC
Thermal & Structure Division
5. Means - ATC - Louvres
• Purpose– dumps more/less power to space– accommodate extreme variation of
energy• internal power• solar fluxes (interplanetary S/C)
– with little temperature change– save heater power
• Principle– blades covering a standard radiator– 16 blades on bearings rotates– opens/closes radiator to deep space
• variation of IR emittance ε– actuator: bi-metallic spring sensing
the radiator temperature
radiator(high ε)
bi-metallic springhousing (low ε)
frame(low ε)
blades(low ε)
S/C radiator
bearings
θ
S/C radiator
actuator blades
bearings bearings
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SME04, 25jun04, [email protected] 61 of 66ESTEC
Thermal & Structure Division
5. Means - ATC - LouvresLouvre on CASSINI-HUYGENS
SENER Louvre on ROSETTA* PFM
*without Solar Panels
louvre
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SME04, 25jun04, [email protected] 62 of 66ESTEC
Thermal & Structure Division
5. Means - ATC - Heaters
• Purpose– additional source of heat inside S/C
• replace power when unit is switched-off• warm up dormant units prior to swon• control temperature and gradient
line in
line out
kapton
metal run
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SME04, 25jun04, [email protected] 63 of 66ESTEC
Thermal & Structure Division
5. Means - ATC - Heaters
ROSETTA FM Heaters
PCUheaters
Battery 2
Battery 3
ROSETTA FM ROSINA DPU
heaters
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SME04, 25jun04, [email protected] 64 of 66ESTEC
Thermal & Structure Division
5. Means - ATC - HeatersROSETTA FM Thruster 12A
self-redundantheaters
FCV
ROSETTA FM OSIRIS PEM-H
glue
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SME04, 25jun04, [email protected] 65 of 66ESTEC
Thermal & Structure Division
5. Means - ATC - Heat Pipes
• Purpose– transport heat by convection with small ∆T– avoid temperature gradients
• Principle– liquid vaporizes at evaporator– gas flows to cold end– gas condensates at cold end– liquid returns by capillary forces
evaporator condenser
Qin Qout
adiabatic section
vapourliquid
liquid
groove
Grooved Heat Pipe
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SME04, 25jun04, [email protected] 66 of 66ESTEC
Thermal & Structure Division
5. Means - ATC - Heat Pipes
Telecom Panel Heat Pipe (Swales)
Ø 12 mm
bi-tube
saddle