Conduction
Convection
Radiation
None of these
B. Convection
Same
More
Less
Depends on other factors
-1/3
-2/3
1
-1
Directly proportional to thermal conductivity
Inversely proportional to density of substance
Inversely proportional to specific heat
All of the above
h = k/ ρS
h = ρS/k
h = S/ρk
h = kρ/S
Conduction
Convection
Radiation
Conduction and convection
Iron
Lead
Concrete
Wood
Face area
Time
Thickness
Temperature difference
Stanton number
Biot number
Peclet number
Grashoff number
6
9
27
81
Black body
Grey body
Opaque body
White body
Nature of the body
Temperature of the body
Type of surface of the body
All of these
Varies with temperature
Varies with the wave length of incident ray
Varies with both
Does not vary with temperature and wave length of the incident ray
Thermometer
Thermistor
Thermocouple
None of these
Conduction
Free convection
Forced convection
Radiation
Increase
Decrease
Remain unaffected
May increase/decrease depending on temperature and thickness of insulation
0.002
0.02
0.01
0.1
It is impossible to transfer heat from low temperature source to t high temperature source
Heat transfer by radiation requires no medium
All bodies above absolute zero emit radiation
Heat transfer in most of the cases takes place by combination of conduction, convection and radiation
Change vapour into liquid
Change liquid into vapour
Increase the temperature of a liquid or vapour
Convert water into steam and superheat it
Increases
Decreases
Remain constant
May increase or decrease depending on temperature
Increases
Decreases
Remain constant
May increase or decrease depending on temperature
Radiant heat is proportional to fourth power of absolute temperature
Emissive power depends on temperature
Emissive power and absorptivity are constant for all bodies
Ratio of emissive power to absorptive power for all bodies is same and is equal to the emissive power of a perfectly black body.
0
0.5
0.75
1
More than those for liquids
Less than those for liquids
More than those for solids
Dependent on the viscosity
Stanton number
Nusselt number
Biot number
Peclet number
Radiators in automobile
Condensers and boilers in steam plants
Condensers and evaporators in refrigeration and air conditioning units
All of the above
Q = [2πlk (T₁ - T₂)]/2.3 log (r₂/r₁)
Q = 2.3 log (r₂/r₁)/[2πlk (T₁ - T₂)]
Q = [2π (T₁ - T₂)]/2.3 lk log (r₂/r₁)
Q = = 2πlk/2.3 (T₁ - T₂) log (r₂/r₁)
Conduction
Free convection
Forced convection
Radiation
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.
Their atoms collide frequently
Their atoms are relatively far apart
They contain free electrons
They have high density
Velocity reduction method
Equal friction method
Static regains method
Dual or double method