A thin sheet of glass is used on the roof of a green- house and is irradiated as shown The irradiation comprises the total solar flux G s , the flux G a t m due to atmospheric emission (sky radiation), and the flux Gi due to emission from interior surfaces. The fluxes G a t m and G i are concentrated in the far IR region λ ≥ 8 μ m .The glass may also exchange energy by convection with the outside and inside atmospheres. The glass may be assumed to be totally transparentfor λ < 1 μ m ( τ λ = 1.0 for λ < 1 μ m ) and opaque,with α λ = 1.0 for λ ≥ 1 μ m . (a) Assuming steady-state conditions, with all radiative fluxes uniformly distributed over the sur- faces and the glass characterized by a uniform temperature T g , write an appropriate energy balance for a unit area of the glass. (b) For T g = 27 ∘ C , h o = 10 W/m 2 ⋅ K , G s = 1100 W/m 2 , T ∞ , o = 24 ∘ C , h o = 55 W/m 2 ⋅ K , G a t m = 250 W/m 2 , and G i = 440 W/m 2 , calculate the temperature of the greenhouse ambient air, T ∞ , i .
A thin sheet of glass is used on the roof of a green- house and is irradiated as shown The irradiation comprises the total solar flux G s , the flux G a t m due to atmospheric emission (sky radiation), and the flux Gi due to emission from interior surfaces. The fluxes G a t m and G i are concentrated in the far IR region λ ≥ 8 μ m .The glass may also exchange energy by convection with the outside and inside atmospheres. The glass may be assumed to be totally transparentfor λ < 1 μ m ( τ λ = 1.0 for λ < 1 μ m ) and opaque,with α λ = 1.0 for λ ≥ 1 μ m . (a) Assuming steady-state conditions, with all radiative fluxes uniformly distributed over the sur- faces and the glass characterized by a uniform temperature T g , write an appropriate energy balance for a unit area of the glass. (b) For T g = 27 ∘ C , h o = 10 W/m 2 ⋅ K , G s = 1100 W/m 2 , T ∞ , o = 24 ∘ C , h o = 55 W/m 2 ⋅ K , G a t m = 250 W/m 2 , and G i = 440 W/m 2 , calculate the temperature of the greenhouse ambient air, T ∞ , i .
Solution Summary: The author explains the energy balance equation for a unit area of the glass.
A thin sheet of glass is used on the roof of a green- house and is irradiated as shown
The irradiation comprises the total solar flux
G
s
, the flux
G
a
t
m
due to atmospheric emission (sky radiation), and the flux Gi due to emission from interior surfaces. The fluxes
G
a
t
m
and
G
i
are concentrated in the far IR region
λ
≥
8
μ
m
.The glass may also exchange energy by convection with the outside and inside atmospheres. The glass may be assumed to be totally transparentfor
λ
<
1
μ
m
(
τ
λ
=
1.0
for
λ
<
1
μ
m
)
and opaque,with
α
λ
=
1.0
for
λ
≥
1
μ
m
.
(a) Assuming steady-state conditions, with all radiative fluxes uniformly distributed over the sur- faces and the glass characterized by a uniform temperature
T
g
, write an appropriate energy balance for a unit area of the glass.
(b) For
T
g
=
27
∘
C
,
h
o
=
10
W/m
2
⋅
K
,
G
s
=
1100
W/m
2
,
T
∞
,
o
=
24
∘
C
,
h
o
=
55
W/m
2
⋅
K
,
G
a
t
m
=
250
W/m
2
,
and G
i
=
440
W/m
2
, calculate the temperature of the greenhouse ambient air,
T
∞
,
i
.
A typical car's exterior consists of a thin layer of silica (SiO2) over an opaque painted metal panel.
Silica is transparent in the visible wavelengths but offers high reflectance in the near- to mid-
infrared wavelengths. The plot on the next page depicts the diffuse spectral reflectivity (pa) of the
car's surface:
Spectral reflectivity, P₂
0.8
0.6
0.4
ལ
0.2
0
0.1
1
1
10
Wavelength, λ(μm)
100
If the car's exterior temperature is T₁ = 77°C, determine both the total absorptivity (a) and the total
emissivity (a) of the silica-covered panel. Assume that the Sun's temperature is Tsun = 5800 K.
CONSIDER AM DBJECT COMPOSED OF TWO SMALL METAL PALLETS LOCATED IN (x;Y) = (2:0) AMD (2:2) AND A PIECE OF WIRE STRETCHED BETWEEN (0;-2) AND
(0:0). (A) DRAW THIS OBJECT. SUPPOSE THAT M PHOTOMS ARE FIRED AT EACH X LATERAL POSITION IM a paralleL -RAY COMFIGURATION. FOR SIMPLICITY,
SUPPOSE THAT EACH METAL OBTECT STOPS HALF OF THE PHOTONS THAT TOUCH IT, REGARDLESS OF THE ANGLE AT WHICH IT IS TOUCHED. (B) DRAW THE
NUMBER OF PHOTOMS YOU EXPECT TO SEE ACCORDING TO x FOR Q = 90° C. DRAW THE RADON TRAMSFORM R (x) FOR = p = 90°
Vector Mechanics for Engineers: Statics, 11th Edition
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