Q KA T= ( 1−T2)CODES
5.
q kA T
=
(
1
−
T
2
)
Codes:
A B C D A B C D
Page 81 of 97
(a)
4
1
3
2
(b)
4
5
1
2
(c)
2
1
3
4
(d)
2
5
1
4
IES-22. Match List-I (Law) with List-II (Effect) and select the correct answer
using the code given below the lists:
[IES-2008]
List-I
List-II
A. Fourier's Law
1. Mass transfer
B. Stefan Boltzmann Law
2. Conduction
C. Newton's Law of Cooling
3. Convection
D. Ficks Law
4. Radiation
Codes:
A
B
C
D
A
B
C
D
(a)
3
1
2
4
(b)
2
4
3
1
(c)
3
4
2
1
(d)
2
1
3
4
Planck's LawIES-23. What is the basic equation of thermal radiation from which all other
equations of radiation can be derived?
[IES-2007]
(a) Stefan-Boltzmann equation
(b) Planck’s equation
(c) Wien’s equation
(d) Rayleigh-Jeans formula
IES-24. The spectral emissive power E
λ
for a diffusely emitting surface is:
E
λ
= 0
for λ< 3 μm [IES-1998]
E
λ
= 150 W/m
2
μm
for 3 < λ < 12 μm
E
λ
= 300 W/m
2
μm
for 12 < λ < 25 μm
E
λ
= 0
for λ > 25 μm
The total emissive power of the surface over the entire spectrum is:
(a) 1250 W/m
2
(b) 2500 W/m
2
(c) 4000 W/m
2
(d) 5250 W/m
2
IES-25. The wavelength of the radiation emitted by a body depends upon
(a) The nature of its surface
(b) The area of its surface
[IES-1992]
(c) The temperature of its surface
(d) All the above factors.
Wien Displacement LawIES-26. Match List-I with List-II and select the correct answer using the code
given below the lists:
[IES-2005]
A. Radiation heat transfer
1. Fourier number
B. Conduction heat transfer
2. Wien displacement law
C. Forced convection
3. Fourier law
D. Transient heat flow
4. Stanton number
Codes:
A
B
C
D
A
B
C
D
(a)
2
1
4
3
(b)
4
3
2
1
(c)
2
3
4
1
(d)
4
1
2
3
IES-27. Sun's surface at 5800 K emits radiation at a wave-length of 0.5 μm. A
furnace at 300°C will emit through a small opening, radiation at a
wavelength of nearly
[IES-1997]
(a)
10
μ (b)
5
μ (c)
0.25
μ (d)
0.025
μ
Page 82 of 97
Intensity of Radiation and Lambert's Cosine LawIES-28. Which one of the following statements is correct?
[IES-2007]
For a hemisphere, the solid angle is measured
(a)
In radian and its maximum value is π
(b)
In degree and its maximum value is 180°
(c)
In steradian and its maximum value is 2 π
(d)
In steradian and its maximum value is π
IES-29. Intensity of radiation at a surface in perpendicular direction is equal
to:
[IES-2005; 2007]
(a) Product of emissivity of surface and 1/π
(b) Product of emissivity of surface and π
(c) Product of emissive power of surface and 1/ π
(d) Product of emissive power of surface and π
IES-30. The earth receives at its surface radiation from the sun at the rate of
1400 W/m
2
. The distance of centre of sun from the surface of earth is