An annular fin of thickness t is used as a radiator to dissipate heat for a space power system. The fin is insulated on the bottom and may be exposed to solar irradiation G s . The fin is coated with a diffuse, spectrally selective material whose spectral reflectivity is specified Heat is conducted to the fin through a solid rod of radius r , and the exposed upper surface of the fin radiates to free space, which is essentially at absolute zero temperature. (a) If conduction through the rod maintains a fin base temperature of T ( r i ) = T b = 400 k and the fin efficiency is 100%, what is the rate of heat dissipation for a fin of radius r o = 0.5 m ? Consider two cases, one for which the radiator is exposed to the sun with G s = 1000 W/m 2 and the other with no exposure ( G s = 0 ) . (b) In practice, the fin efficiency will be less than 100% and its temperature will decrease with increasing radius. Beginning with an appropriate control volume, derive the differential equation that determines the steady-state, radial temperature distribution in the fin. Specify appropriate boundary conditions.
An annular fin of thickness t is used as a radiator to dissipate heat for a space power system. The fin is insulated on the bottom and may be exposed to solar irradiation G s . The fin is coated with a diffuse, spectrally selective material whose spectral reflectivity is specified Heat is conducted to the fin through a solid rod of radius r , and the exposed upper surface of the fin radiates to free space, which is essentially at absolute zero temperature. (a) If conduction through the rod maintains a fin base temperature of T ( r i ) = T b = 400 k and the fin efficiency is 100%, what is the rate of heat dissipation for a fin of radius r o = 0.5 m ? Consider two cases, one for which the radiator is exposed to the sun with G s = 1000 W/m 2 and the other with no exposure ( G s = 0 ) . (b) In practice, the fin efficiency will be less than 100% and its temperature will decrease with increasing radius. Beginning with an appropriate control volume, derive the differential equation that determines the steady-state, radial temperature distribution in the fin. Specify appropriate boundary conditions.
Solution Summary: The author explains the rate of heat dissipation for a fin if radiator is exposed to the sun with solar radiation.
An annular fin of thickness t is used as a radiator to dissipate heat for a space power system. The fin is insulated on the bottom and may be exposed to solar irradiation
G
s
. The fin is coated with a diffuse, spectrally selective material whose spectral reflectivity is specified
Heat is conducted to the fin through a solid rod of radius
r
, and the exposed upper surface of the fin radiates to free space, which is essentially at absolute zero temperature.
(a) If conduction through the rod maintains a fin base temperature of
T
(
r
i
)
=
T
b
=
400
k
and the fin efficiency is 100%, what is the rate of heat dissipation for a fin of radius
r
o
=
0.5
m
? Consider two cases, one for which the radiator is exposed to the sun with
G
s
=
1000
W/m
2
and the other with no exposure
(
G
s
=
0
)
.
(b) In practice, the fin efficiency will be less than 100% and its temperature will decrease with increasing radius. Beginning with an appropriate control volume, derive the differential equation that determines the steady-state, radial temperature distribution in the fin. Specify appropriate boundary conditions.
A horizontal opaque flat plate is well insulated on the edges and the lower surface. The top surface has an area of 5 m2, and it experiences uniform irradiation at a rate of 5000 W. The plate absorbs 4000 W of the irradiation, and the surface is losing heat at a rate of 500 W by convection. If the plate maintains a uniform temperature of 350 K, determine the absorptivity, reflectivity, and emissivity of the plate.
Pravinbhai
Wien's law is stated as follows: AmT = C, where C is 2898 μmK and Am is the wavelength at which the emissive
power of a black body is maximum for a given temperature T. The spectral hemispherical emissivity (Ex) of a surface
is shown in the figure below (1Å= 10-¹0m). The temperature at which the total hemispherical emissivity will be
highest is
K (round off to the nearest integer).
Ext
n
5000
6000 7000 (A)
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