In the central receiver concept of solar energy collection, a large number of heliostats (reflectors) provide a concentrated solar flux of q s " = 80 , 000 W/m 2 to the receiver, which is positioned at the top of a tower. The receiver wall is exposed to the solar flux at its outer surface and to atmospheric air for which T ∞ , o = 300 K and h o = 25 W/m 2 ⋅ K . The outer sur- face is opaque and diffuse, with a spectral absorptivity of α λ = 0.9 for λ <3 μ m α λ = 0.2 for λ > 3 μ m . The inner surface is exposed to a working fluid (a pressurized liquid) for which T ∞ , i = 700 K and h i = 1000 W/m 2 ⋅ K . The outer surface is also exposed to surroundings for which T s u r = 300 K . If the wall is fabricated from a high-temperature material for which K=15W/m ⋅ K ,what is the minimum thickness L needed to ensure that the outer surface temperature does not exceed T s , o = 1000 K ? What is the collection efficiency associated with this thickness?
In the central receiver concept of solar energy collection, a large number of heliostats (reflectors) provide a concentrated solar flux of q s " = 80 , 000 W/m 2 to the receiver, which is positioned at the top of a tower. The receiver wall is exposed to the solar flux at its outer surface and to atmospheric air for which T ∞ , o = 300 K and h o = 25 W/m 2 ⋅ K . The outer sur- face is opaque and diffuse, with a spectral absorptivity of α λ = 0.9 for λ <3 μ m α λ = 0.2 for λ > 3 μ m . The inner surface is exposed to a working fluid (a pressurized liquid) for which T ∞ , i = 700 K and h i = 1000 W/m 2 ⋅ K . The outer surface is also exposed to surroundings for which T s u r = 300 K . If the wall is fabricated from a high-temperature material for which K=15W/m ⋅ K ,what is the minimum thickness L needed to ensure that the outer surface temperature does not exceed T s , o = 1000 K ? What is the collection efficiency associated with this thickness?
Solution Summary: The author explains the minimum thickness L and the collection efficiency associated with this thickness.
In the central receiver concept of solar energy collection, a large number of heliostats (reflectors) provide a concentrated solar flux of
q
s
"
=
80
,
000
W/m
2
to the receiver, which is positioned at the top of a tower.
The receiver wall is exposed to the solar flux at its outer surface and to atmospheric air for which
T
∞
,
o
=
300
K
and h
o
=
25
W/m
2
⋅
K
. The outer sur- face is opaque and diffuse, with a spectral absorptivity of
α
λ
=
0.9
for
λ
<3
μ
m
α
λ
=
0.2
for
λ
>
3
μ
m
. The inner surface is exposed to a working fluid (a pressurized liquid) for which
T
∞
,
i
=
700
K
and h
i
=
1000
W/m
2
⋅
K
. The outer surface is also exposed to surroundings for which
T
s
u
r
=
300
K
. If the wall is fabricated from a high-temperature material for which
K=15W/m
⋅
K
,what is the minimum thickness L needed to ensure that the outer surface temperature does not exceed
T
s
,
o
=
1000
K
? What is the collection efficiency associated with this thickness?
Can you solve it analytically using laplace transforms and with Matlab code as well please. Thank You
Can you solve it analytically using laplace transforms and with Matlab code as well please. Thank You.
Q11. Determine the magnitude of the reaction force at C.
1.5 m
a)
4 KN
D
b)
6.5 kN
c)
8 kN
d)
e)
11.3 KN
20 kN
-1.5 m-
C
4 kN
-1.5 m
B
Mechanical engineering, No
Chatgpt.
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