Solar collectors - ČVUT Fakulta...
Transcript of Solar collectors - ČVUT Fakulta...
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Solar collectors
types
efficiency
application
statistics
AES-L2
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Photothermal conversion
collecting surface (collector)
surface absorbing solar radiation which converts to heat
accummulation (heat storage)
storing the solar heat gains for further use
(storage tank, wall, mass in the building space, ...)
consumer
hot water, heating, cooling, ...
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Solar collector
Pipes with heat transfer fluid
Transparent cover - glazing
Absorber
Thermal insulation
Collector frame
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Solar collectors
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Solar air collectors
heat transfer fluid is air
heats from outer surface of
absorber
low heat capacity, high
flowrates, large dimensions
high auxilliary electricity use
applications:
agriculture – drying
residental – heating of
ventilation air
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Solar air collectors
Box
Frame
Glazing
Insulation
Finned absorber
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Solar air collectors
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Solar air collectors
integration into roof
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Solar liquid collectors
liquid as heat transfer fluid
(water, antifreeze, oil, etc.)
energy absorbed at surface is
removed by heat transfer liquid
flowing inside pipes of
absorber
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Solar collectors
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Unglazed solar collectors
temperature level < 40 °C
seasonal applications, swimming pools
strongly dependent on ambient conditions
(temperature, wind)
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Solar collectors
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Flat plate covered solar collectors
1 frame
2 sealing
3 transparent cover
4 thermal insulation
5 absorber
6 pipe register
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Flat plate solar collectors
suitable for building envelope integration
roof
facade
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Solar collectors
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Vacuum flat plate solar collectors
underpressure to reduce heat loss (absolute pressure 1 to 10 kPa)
load upon flat cover glazing (pillars)
need for shading the radiation heat trasfer
to back side (IR reflectors)
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Solar collectors
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Vacuum tube solar collectors
single vacuum tube
flat absorberdouble vacuum tube (Sydney)
cylindric absorber
high vacuum 1 mPa
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Vacuum tube solar collectors
Single vacuum tube
with flat absorber
direct flow (DF)
high quality heat transfer from absorber into fluid
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Vacuum tube solar collectors
Single vacuum tube
with flat absorber
heat pipe (HP)
high quality heat transfer from absorber to evaporator part
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Vacuum tube solar collectors
source: Viessmann
heat pipe
direct flow
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Vacuum tube solar collectors
single vacuum tube
flat absorberdouble vacuum tube (Sydney)
cylindric absorber
high vacuum 1 mPa
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Vacuum tube solar collectors
Double vacuum Sydney tube
with cylindric absorber
direct flow (DF)
with a contact fin
heat transfer fin between absorber tube and pipe register needed!
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Vacuum tube solar collectors
Double vacuum Sydney tube
with cylindric absorber
heat pipe (HP)
with a contact fin
heat transfer fin between absorber tube and evaporator needed!
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Vacuum tube (Sydney) solar collectors
contact fin connection DF pipes Sydney tubes
reflector
source: OPC
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Vacuum tube (Sydney) solar collectors
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Vacuum tube (Sydney) solar collectors
barium absorbs gases and
changes colour
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Vacuum tube (Sydney) solar collectors
The getter material is held inactive in a reservoir during
assembly, then heated and evaporated after initial
evacuation. The vaporized getter, usually a volatile
metal, instantly reacts with any residual gas, then
condenses on the cool walls of the tube in a thin coating,
the getter mirror, which continues to absorb gas.
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Vacuum tube (Sydney) solar collectors
vacuum insulation = snow or frost removed very slowly
snow accummulation: problematic use of reflectors
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Flat plate collectors and defrosting
heat loss allows collector operation even in periods of snow cover
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Tube collector with a heat pipe
heat removed by evaporator
of heat pipe
solar energy
absorbed at
absorber
heat removed to heattransfer fluid
condenser
evaporator
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Tube collector with a heat pipe
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Tube collector with a heat pipe
dry connection
condenser placed in a slot
slot washed by heat transfer fluid
source: Viessmann
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Tube collector with a heat pipe
wet connection
condenser of heat pipe directly
washed by heat transfer fluid
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Tube collector with a reflector
specular reflection
diffuse reflection
durability of optical
quality of reflector
snow and ice
accummulation, tube
destruction
increase of
collector active
area (aperture)
compound parabolic reflector (CPC)
flat reflector
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Concentrating solar collectors
concentration of direct solar radiation
reflection (mirrors) x refraction (lenses)
linear focus
parabolic reflector
Winston collector (trough form)
collector with a Fresnel lens
point focus
paraboloid reflector
heliostats
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Concentrating solar collectors (reflection)
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Collector with Fresnel lenses (refraction)
combined active and
passive component
source: ENKI
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Principle and balance of solar collector
Heat loss through
glazing
Reflection
at absorberReflection at glazing
Incident solar
radiation
Heat loss through
side and back wall
Heat removal by fluid
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Solar collector glazing
single glazing
low-iron glass, solar glass
low absorbance of solar radiation
antireflective coatings
reduction of reflection at interface glass-air
prismatic glass (pyramidal texture)
increase of transmittance at high angles
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Reflection loss
reflection at each interface glass-air 4 % (normal)
independent on thickness
100 % 91 %
solar glass
4 % + 4 %
1 %
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Antireflection (AR) coatings
reflection reduced to 1,5 % at each interface glass-iron
coating with low refraction index
100 % 96 %
solar glass with
double AR3 %
1 %
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Solar collector absorber
radiation properties for athermanous bodiesAthermanous body is such a body through which any heat radiation cannot pass.
absorptance a + reflectance r = 1
for given wavelength l apply: absorptance al = emittance el
perfect black body: a = 1, r = 0 for all wavelengths
perfect white body: a = 0, r = 1 for all wavelengths
grey body 0 < a = al < 1, r = 1 – a for all wavelengths
selective body 0 < al < 1, rl = 1 – al aSOL ≠ eIR
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Absorber selectivity
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Absorber selectivity
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Absorber selectivity
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Absorber selectivity
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Absorber selectivity
solar radiation
spectrum (Sun)
infrared radiation
spectrum (absorber)
ideal r = 0, e = a = 1
ideal r = 1, a = e = 0
refl
ecta
nce
[-]
ideal selective
absorber
black chrome
Ni-AlO3
wavelength
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Selective surfaces
galvanic
electrochemical process
a = 0,93 – 0,96, e = 0,10 – 0,16
ceramic-metal (cermet)
sputtering, physical vapour deposition
process, high quality surfaces
a = 0,95, e = 0,05
paints
considerably worse
a = 0,92, e = 0,85
material goes from a condensed phase to a vapor phase
and then back to a thin film condensed phase
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Efficiency of solar collector
t ... glazing transmittance for solar radiation [-]
a ... absorber absorptance for solar radiation [-]
U ... heat loss coefficient [W/m2.K]
tabs ... mean absorber temperature [°C]
te ... ambient temperature [°C]
G
ttU eabs
ta
optical efficiency
heat loss
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Simple calculation
collector C1 C2
transmittance of collector glazing: 0,90 0,90
absorptance of collector absorber: 0,90 0,90
front U-value 6 W/m2K 3 W/m2K
back U-value 1 W/m2K 1 W/m2K
calculate efficiency for given conditions:
te = 10 °C
G = 800 W/m2
tabs = 20 °C 80 °C
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Simple calculation
800
10)13(9,09,0
abst
800
10)16(9,09,0
abst
Collector 1 Collector 2
0,0
0,2
0,4
0,6
0,8
1,0
0 0,02 0,04 0,06 0,08 0,1 0,12
(t abs - t e)/G [m2K/W]
[
-]
C1
C2
G
ttU eabs
ta
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Efficiency of solar collector
~ (1-ta)
~ U(tabs-te)
optical loss
heat loss
efficiency
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Efficiency of solar collector
F’ ... efficiency factor > 0.90
depends on geometry and thermal properties of absorber
………..quality heat transfer from the absorber to the heat transfer fluid
tm ... mean fluid temperature
tm = (tk1+tk2)/2
G
ttU eabs
ta
G
ttUF emta '
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Heat transfer from absorber surface
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Efficiency factor F’
depends on
geometry of absorber:
pipe distance, pipe dimension, thickness of pipe-absorber
bond, absorber thickness
physical properties of absorber:
thermal conductivity of absorber, thermal conductance of the
bond pipe-absorber
flow regime in pipes: heat transfer from pipe wall to fluid
total heat loss coefficient of collector U
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Determination of heat output by testing
)( k1k2k ttcMQ
)( k1k2k ttcMQ
tk1
tk2G
M.
kAG
Q
k
efficiency [-]
heat output [W]
solar collector power
tested at clear sky, G > 700 W/m2, normal incidence, w > 3 m/s
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Efficiency characteristic
0,0
0,2
0,4
0,6
0,8
1,0
0,00 0,05 0,10 0,15 0,20
(t m - t e)/G [m2.K/W]
[-]
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Efficiency characteristic = f (tm – te)
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Reference collector area Ak
gross area: AG
aperture area: Aa
absorber area: AA
k
k
AG
Q
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Reference collector area Ak
AA AA
AA
Aa Aa Aa
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Reference collector area Ak
aperture: comparison of collector quality, construction
gross area: decision on potential for given application (limited space on roof)
Aa = 0,9 AG Aa = 0,75 AG Aa = 0,6 AG Aa = 0,8 AG
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Efficiency characteristic
G
tta
G
tta emem
2
210
0 „optical“ efficiency [-], better: zero-loss efficiency
a1 linear heat loss coefficient [W/(m2.K)]
„related to difference between absorber and ambient temperature“
a2 quadratic heat loss coefficient [W/(m2.K2)] „simplified approach for the radiation losses“
values 0, a1, a2 related to reference area Ak (aperture is preferred)
coefficients are given by producer, supplier or testing institute based
on test report in accordance to EN 12975-2
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Theory x testing
0 = F’ta zero-loss efficiency
a1+a2(tm - te) = F’U heat loss coefficient
G
tta
G
tta emem
2
210
G
ttUFF em
''ta
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Typical coefficients *)
Collector type0 a1 a2
- W/(m2K) W/(m2K2)
Unglazed 0.85 20 -
Glazed with nonselective absorber 0.75 6.5 0.030
Glazed with selective absorber 0.78 4.2 0.015
Vacuum single tube (flat absorber) 0.75 1.5 0.008
Vacuum tube Sydney 0.65 1.5 0.005
*) referenced to aperture area
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Heat output (power) of solar collector
GAQ kpeakk 0,
solar collector power (normal incidence, clear sky)
installed (nominal) power
– for defined conditions (according to ESTIF):
G = 1000 W/m2 te = 20 °C tm = 50 °C
peak power (without heat loss)
])()([ 2210 ememkkk ttattaGAGAQ
G = 1000 W/m2
0 „optical“ efficiency [-], a1 linear heat loss c. [W/(m2.K)] a2 quadratic heat loss c. [W/(m2.K2)]
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0
400
800
1200
1600
0 50 100 150
Qk
[W]
(tm - te) [K]
G = 1000 W/m2
Heat output (power) of solar collector
installed power
peak power
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Efficiency and power calculation
flat-plate vacuum tube
0,a 0,75 0,65 -
a1,a 3,5 1,5 W/m2K
a2,a 0,015 0,005 W/m2K2
AG 4 m2
Aa 3,6 2,4 m2
calculation of daily efficiency for April,
Prague city, slope 45°, azimuth 45°
GT,m W/m2
te,s °C
tk,m °C
473
12,1
40
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Efficiency and power calculation
flat-plate vacuum tube
k -
Qk,m W
Qk,day kWh/day
mT
semk
mT
semkk
G
tta
G
tta
,
2,,
2
,
,,10
dayTkkdayk HAQ ,,
mTkkmk GAQ ,,
0,52 0,55
884 628
6,8 4,8
dayTH , 3.64 kWh/m2.day
daily solar irradiation difdayTrthdayTrdayT HHH ,,,,, 1 tt
mean daily solar irradiance
t
thdayTmT
HG
t
,,,
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Nominal conditions (ESTIF)
flat-plate vacuum tube
G 1000 W/m2
te,s 20 °C
tm 50 °C
k
Qk,nom W
Qk,peak W
GAQ kpeakk 0,
0,63 0,60
2273 1441
2700 1560
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Solar collector / applications
0.0
0.2
0.4
0.6
0.8
1.0
0 20 40 60 80 100 120 140 160t m - t e [K]
[-]
unglazed flat/plate selective
single vacuum tube Sydney vacuum tube
pools hot water & space heating
process heat high temperature
industrial applications
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Solar collectors in the World
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Solar collectors installed (valid for 2015)
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Solar collectors installed (valid for 2015)
world
Europe
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Solar collectors installed (valid for 2015)
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Solar collectors installed (valid for 2015)
per 1000 inhabitants
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Solar collectors new installations (2015)