α = 1, ρ = 0 and τ = 0
α = 0, ρ = 1 and τ = 0
α = 0, ρ = 0 and τ = 1
α + ρ = 1 and τ = 0
D. α + ρ = 1 and τ = 0
The total radiation from a black body per second per unit area is directly proportional to the fourth power of the absolute temperature
The wave length corresponding to the maximum energy is proportional to the absolute temperature
The ratio of the emissive power and absorptive power of all bodies is the same and is equal to the emissive power of a perfectly black body
None of the above
P = 0, x = 0 and a = 1
P=1, x = 0, and a = 0
P = 0, T= 1, and a = 0
X = 0, a + p = 1
Directly proportional to the surface area of the body
Directly proportional to the temperature difference on the two faces of the body
Dependent upon the material of the body
All of the above
Change vapour into liquid
Change liquid into vapour
Increase the temperature of a liquid or vapour
Convert water into steam and superheat it
Stanton number
Nusselt number
Biot number
Peclet number
A dimensionless parameter
Function of temperature
Used as mathematical model
A physical property of the material
The time taken to attain the final temperature to be measured
The time taken to attain 50% of the value of initial temperature difference
The time taken to attain 63.2% of the value of initial temperature difference
Determined by the time taken to reach 100°C from 0°C
m²/hr
m²/hr °C
kcal/m² hr
kcal/m. hr °C
RN = hl/k
RN = μ cp/k
RN = ρ V l /μ
RN = V²/t.cp
Convection
Radiation
Forced convection
Free convection
1 : 1
2 : 1
1 : 2
4 : 1
More than those for liquids
Less than those for liquids
More than those for solids
Dependent on the viscosity
Same
Less
Greater
None of these
Maximum
Minimum
Zero
None of these
Thermal conductivity to the equivalent thickness of the film of fluid
Temperature drop through the films of fluids to the thickness of film of fluids
Thickness of film of fluid to the thermal conductivity
Thickness of film of fluid to the temperature drop through the films of fluids
Grashoff number
Biot number
Stanton number
Prandtl number
tm = (Δt1 - Δt2)/ loge (Δt1/Δt2)
tm = loge (Δt1/Δt2)/ (Δt1 - Δt2)
tm = tm = (Δt1 - Δt2) loge (Δt1/Δt2)
tm = loge (Δt1 - Δt2)/ Δt1/Δt2
Function of temperature
Physical property of a substance
Dimensionless parameter
All of these
A grey body is one which absorbs all radiations incident on it.
At thermal equilibrium, the emissivity and absorptivity are same.
The energy absorbed by a body to the total energy falling on it, is called emissivity.
A perfect body is one which is black in colour.
Higher
Lower
Same
Depends on the area of heat exchanger
Thermal conductivity
Thermal diffusivity
Density
Dynamic viscosity
Directly proportional to the surface area
Directly proportional to the difference of temperatures between the two bodies
Either (A) or (B)
Both (A) and (B)
Glass
Water
Plastic
Air
α = 1, ρ = 0 and τ = 0
α = 0, ρ = 1 and τ = 0
α = 0, ρ = 0 and τ = 1
α + ρ = 1 and τ = 0
The heat transfer in liquid and gases takes place according to convection.
The amount of heat flow through a body is dependent upon the material of the body.
The thermal conductivity of solid metals increases with rise in temperature
Logarithmic mean temperature difference is not equal to the arithmetic mean temperature difference.
Black bodies
Polished bodies
All coloured bodies
All of the above
0.1
0.23
0.42
0.51
Thermal resistance
Thermal coefficient
Temperature gradient
Thermal conductivity
First law of thermodynamics
Newton's law of cooling
Newton's law of heating
Stefan's law
P = 0, x = 0 and a = 1
P=1, x = 0 and a = 0
P = 0, x = 1 and a = 0
X = 0, a + p = 1 Where a = absorptivity, p = reflectivity, X = transmissivity.