selective coatings
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Selective absorbers
Dr. Ángel Morales
Optical Coatings Technology Lab.
Unit of Solar Concentrating Systems
Plataforma Solar de Almería PSA
CIEMAT
Solar absorbers
• Solar absorbers are the responsible to
collect solar radiation.
• Solar radiation produces absorber heating
that is transferred to the substrate.
• Collected energy is exhausted by heat
transfer fluid.
• Thermal losses: conduction-convection
with air and IR emission.
Thermal losses
• Conduction when a material is in direct
contact with other.
• Convection when a material is in contact
with a moving fluid.
• Radiation when a material is at higher
temperature than surroundings.
Absorber thermal losses
• Absorber conduction-convection losses
are reduced:
– Glass covers
– Vacuum between glass and absorber.
• Absorber IR losses????
– Selective absorbers
Solar and IR radiation
• Absorber collects solar radiation and some
energy is emitted as infrared radiation.
0
0,1
0,2
0,3
0,4
0,5
0,6
0,7
0,8
0,9
1
0 2 4 6 8 10Wavelength (microns)
No
rma
lis
ed
em
iss
ion
673 K
5673 K
Optical parameters
Solar radiation
Reflectance (R)
Transmittance (T)
Absorption (a)
1 aTR
Spectral selectivity
• Spectral selectivity:
– Materials that present different behavior in
two broad spectral ranges.
• Examples:
– Glass
– Transparent conductor oxides (TCO)
– Solar selective absorbers
Glass selectivity
• Glass is transparent to solar radiation and
it absorbs far IR radiation
Transparent conductor oxide
• TCO is transparent to visible radiation and
it reflects mid and far IR
Optical properties
1 aTR
1 TR
a Kirchoff’s law
1aR R1a
1R R1
Selective absorber
m
m
m
mhem
s
dGAM
GdAMR
a
5,2
3,0
5,2
3,0
5.1
5.1)1(
m
mbb
m
mbbhem
T
dTi
dTiR
25
3,0
25
3,0
),(
),()1(
Solar absorptance Thermal emittance
Solar absortance and thermal
emittance
Absorption edge location
Maximum solar absorptance (absorption edge position) vs. absorber
temperature and a fixed thermal emittance.
Tª(ºC) =0,01 =0,05 =0,10 =0,15
5 99,9(4,81) 99,9(6,27) 99,9(7,41) 99,9(8,15)
100 99,7(3,87) 99,9(5,06) 99,9(5,96) 99,9(6,55)
200 99,0(3,05) 99,9(3,99) 99,9(4,70) 99,9(5,17)
300 98,8(2,52) 99,2(3,30) 99,7(3,88) 99,9(4,26)
400 96,8(2,14) 98,8(2,80) 99,2(3,30) 99,4(3,63)
500 95,3(1,87) 98,5(2,44) 98,9(2,87) 99,0(3,16)
Absorptance vs. emittance
• Increasing solar absorptance produces higher thermal
emittance.
• For non concentrating systems, solar absorptance is
more critical than thermal emittance. As temperature
increases, emittance contribution is higher.
– Collection area equal than emission area.
• For high temperature applications, increasing
concentration makes solar absorptance to be more
critical than thermal emittance.
• Collection area higher than emission area.
Absorption edge location
Solar absorptance and thermal emittance (400ºC) for two absorbers with different
absorption edge position and slope.
Solar selective materials
• There is no any material with good solar
selectivity:
– Metals have low emittance and low solar
absorptance.
– Semiconductors and metal oxides have
moderate absortance and high thermal
emittance.
– It is necessary to combine two materials to
obtain good solar selectivity.
Selective absorber types
• Absorber/metal tandem
• Absorber/metal tandem with AR layer
• Optical trapping
• Metal/dielectric composite materials
(Cermets)
• High performance selective absorbers
Infrared reflectors
• Metals such as Cu, Al, Ag, W, Mo:
– Good IR reflectance.
– Low thermal stability in air.
• Noble metals such as Au, Pt:
– Au RIR,=0,98, Pt RIR=0,93.
– Good IR reflectance.
– High thermal stability in air.
– Very thin layers are needed (50 nm)
Metals emissivity
200 300 400 500 600 700 800 900 1000 1100 0
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0.08
HEMISPHÉRICAL TOTAL EMISSIVITY
FOR SEVERAL METALS
TEMPERATURE (K)
HE
MIS
PH
ÉR
ICA
L T
OT
AL
EM
ISS
IVIT
Y
Ag Cu Al Mo Au Pt
Absorber /IR reflector tandem
• Simplest solar absorber: metal oxide layer
over an infrared reflective metal layer.
• Low absorptance (<0.90) due to high
reflectance losses on oxide layer.
2. Absorber layer
3. Infrared reflector
Metallic substrate
2. Absorber layer
3. Infrared reflector
Metallic substrate
Antireflective layers
1. Antireflective coating
2. Absorber layer
3. Infrared reflector
Metallic substrate
1. Antireflective coating
2. Absorber layer
3. Infrared reflector
Metallic substrate
• AR layers: refractive index between air and metal oxide
layer.
• Solar absorptance increases from 0.90 to 0.96
• Thickness:
Optical trapping
• Increasing average roughness of substrate, solar
absorptance and thermal emittance are higher.
• Actually, it is not used because thermal emittance is too
high and coatings adhesion and durability are poorer.
d
<d d
Metal/dielectric composites (Cermets)
• Cermet: metal particles dispersed in a dielectric matrix.
• High solar absorptance and low thermal emittance.
• Two types: homogenous or graded.
Metal particles Dielectric matrix
GRADED ABSORBER CERMET
Metal particles Dielectric matrix
HOMOGENEOUS ABSORBER CERMET
Solar radiation (optical trapping)
IR radiation (no optical trapping)
LMVF/HMVF cermets
• Increasing metal volume fraction:
– Higher absortance
– Higher reflectance
– Higher emittance
• It is necessary to optimize metal volume
fraction, in both cermet layers, to obtain
best optical properties.
High performance absorbers
• Absorbing layer composed of low and high metal volume
fraction (LMVF/HMVF cermets).
• Diffusion barrier to avoid infrared reflector diffusion into
metal substrate.
2. Absorber layer
3. Infrared reflector
Metallic substrate
1. Antireflective coating
3. HMVF cermet
4. Infrared reflector
Metallic substrate
5. Difussion barrier
2. LMVF cermet
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90
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250 500 750 1000 1250 1500 1750 2000 2250 2500
Hem
isp
he
ric
al re
flecta
nc
e
Wavelength (nm)
Effect of absorbing layer
thickness
AR
absorber
IR reflector
d1 (a=0.937)
d2 (a=0.941) d2>d1
absorber
Effect of AR layer thickness
d1 (a=0.941)
d2 (a=0.947)
d3 (a=0.945) d3>d2>d1
AR (d1,d2,d3)
absorber
IR reflector
Selective absorber types
• Different absorber for each application:
– flat collectors and low temperature vacuum
systems T<150ºC).
– CPC systems for industrial heat (250-350ºC)
– CPC for electricity production (400-550ºC)
– Central receivers (500-100ºC).
Low temperature absorber
Cu or Al
SiO2 AR layer
TiNOx
SnO2 AR layer
• a=0.95, (100C)=0.08
• Stable in air at 200ºC
CPC systems for industrial heat
• Black Chrome: a=0.95, 300ºC=0.13
• Thermal stability: 250ºC
Medium temperature absorbers
High temperature absorbers
• Black paints: high solar absorptance and thermal
emittance
• Solar selectivity is reduced. There is no any selective
absorber for this application.
Durability
• Degradation agents:
– Temperature
– Humidity and condensation
• Degradation modes:
– Oxidation of metallic particles in cermets
and/or IR reflectors.
– Peeling, cracking, adhesion problems.
Durability tests
• Low temperature (IEA task X test): – 600h condensation + 40ºC
– 300h at 250ºC
– PC = -a + 0.25x
• Medium temperature (no test): – 300h temperature 50-100ºC higher than operation
– 600h condensation
• High temperature in vacuum (no test): • xh? temperature 50-100ºC higher than operation
Production methods
• Chemical methods: – Electrodeposition
– Anodic oxidation
– Chemical vapor deposition (CVD)
– Spray pyrolysis
– Sol-gel / Dip-coating
• Physical methods: – Evaporation
– Sputtering
Commercial production methods
• Electrodeposition:
– Black chrome.
• Sputtering:
– All commercial coatings are produced by
sputtering (flat collectors and CPC).
– Graded and homogeneous cermets.
• Sol-gel / dip-coating:
– Spinels (mixed metal oxide coatings).
Electrodeposition
• Advantages:
– Low technology requirements
– Very cheap
– Easy scalability for different sizes and shapes
• Disadvantages:
– Chrome is quite poisonous and contaminant.
– No further production new plants
Sputtering
• Advantages: – Any material can be produced.
– Very good reproducibility and homogeneity.
– Price????.
• Disadvantages: – High technology requirements.
– Not easy scalability for different sizes and shapes
with the same machine.
– Price???.
Sputtering
• In a vacuum chamber, a noble gas is introduced.
• It is ionized and accelerated against the target,
using an electric field.
• Material is removed from the target and it is
deposited on the substrate.
• Coating thickness and properties are controlled
by substrate temperature, time and power of
deposition, controlled atmosphere…
Dip-coating technology
• Three steps:
• Precursor solution
preparation (sol-gel or
inorganic metal salts)
• Sample withdrawal at
constant speed
• Thermal treatment to remove
organics and obtain dense
films Tª
1
-
v
cte precursor
solution
2-
3-
heating
system
sample
precursor
solution
preparation
engine
Sol-gel materials
• Metal oxides:
– SiO2, TiO2, Al2O3, …
• Mixed metal oxides:
– SiO2+TiO2, SiO2 +Al2O3
• Cermets:
– SiO2(Me), TiO2(Me)
Dip-coating materials
• Metal oxides:
– Co, Cu, Al, Mn, Al, …
– Mixed metal oxides
• Cermets:
– Al2O3(Pt), Al2O3(Au), TiO2(Au)
• Metals:
– Pt, Au, Pd
• Metal sulphides
– PbS, CdS, CuS
Advantages and disadvantages
• Advantages: – Low technology requirements.
– Very cheap (low cost materials, energy).
– Easy scalability for different sizes and shapes.
– Precursor solutions last years.
• Disadvantages: – Materials produced are limited.
– Production time for multilayer coatings.
– Bankability.
Layer deposition system
• Coating large tubes vertically
implies high height industrial
installations to withdraw tube from
the precursor solution. So, solution
containers must to be in the
ground.
• It is possible to avoid this problem
using a mobile pot patented by
CIEMAT.
• It consists of a cylindrical container
with a centered hole and a tight O-
ring to avoid solution losses.
Coating is performed moving down
the pot along the tube.
v
Low temperature absorber
Aluminum
Absorbing layer
SiO2 AR layer
MnCuOx/SiO2 layer
a=0.954, (100C)=0.045
Stable in air at 350ºC
Industrial heat applications
• a=0.96, (300C)=0.16
• Stable in air at 400ºC
Stainless steel
Absorbing layer
SiO2 AR layer
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250 500 750 1000 1250 1500 1750 2000 2250 2500
Hem
isp
heri
cal
refl
ecta
nce
Wavelength (nm)
CPC (electricity production)
• a=0.96, (400ºC)=0.087
• Stable in air at 500ºC
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Hem
isp
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Wavelength (nm)
Stainless steel
Absorbing layer
SiO2 AR layer
Difussion barrier
Pt reflector
Difussion barrier
CPC (electricity production)
Stainless steel
Absorbing layer
SiO2 AR layer
Difussion barrier
Pt reflector
Difussion barrier
CPC (electricity production)
Silicon dioxide
Diffusion barrier
Diffusion barrier
Platinum reflector
Absorbing layer
AR layer
Central receivers
• Platinum absorber components are stable
at temperatures higher than 1000ºC.
• Thermal durability depends on interlayer
diffusion.
• Increasing platinum and diffusion barriers
thicknesses thermal stability is improved.
• At present, we are testing 700ºC stable
selective absorbers for tube receivers.
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