Fourier equation
Stefan-Boltzmann equation
Newton Reichmann equation
Joseph-Stefan equation
B. Stefan-Boltzmann equation
Below which a gas does not obey gas laws
Above which a gas may explode
Below which a gas is always liquefied
Above which a gas will never liquefied
Fourier equation
Stefan-Boltzmann equation
Newton Reichmann equation
Joseph-Stefan equation
Absolute temperature (T)
I²
F
T
Nature of body
Temperature of body
Type of surface of body
All of the above
Function of temperature
Physical property of a substance
Dimensionless parameter
All of these
The better insulation must be put inside
The better insulation must be put outside
One could place either insulation on either side
One should take into account the steam temperature before deciding as to which insulation is put where
Thermal resistance
Thermal coefficient
Temperature gradient
Thermal conductivity
High thickness of insulation
High vapour pressure
Less thermal conductivity insulator
A vapour seal
Equivalent thickness of film
Thermal conductivity Equivalent thickness of film Specific heat × Viscosity
Thermal conductivity Molecular diffusivity of momentum Thermal diffusivity
Film coefficient × Inside diameter Thermal conductivity
Kirchoffs law
Stefan's law
Wien' law
Planck's law
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
Hr (time)
Sq. m (area)
°C (temperature)
K.cal (heat)
Their atoms collide frequently
Their atoms are relatively far apart
They contain free electrons
They have high density
Parallel flow
Counter flow
Cross flow
All of these
Directly proportional to the thermal conductivity
Inversely proportional to density of substance
Inversely proportional to specific heat
All of the above
Reynold's number
Grashoff's number
Reynold's number, Grashoff's number
Prandtl number, Grashoff's number
Temperature
Thickness
Area
Time
Shorter wavelength
Longer wavelength
Remain same at all wavelengths
Wavelength has nothing to do with it
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
Conduction
Convection
Radiation
None of these
0.1
0.3
0.7
1.7
Q = 2πkr1 r2 (T1 - T2)/ (r2 - r1)
Q = 4πkr1 r2 (T1 - T2)/ (r2 - r1)
Q = 6πkr1 r2 (T1 - T2)/ (r2 - r1)
Q = 8πkr1 r2 (T1 - T2)/ (r2 - r1)
Directly proportional to thermal conductivity
Inversely proportional to density of substance
Inversely proportional to specific heat
All of the above
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.
Nature of the body
Temperature of the body
Type of surface of the body
All of these
Conduction
Convection
Radiation
Conduction and convection
Increases
Decreases
Remain constant
May increase or decrease depending on temperature
Grashoff number
Biot number
Stanton number
Prandtl number
A.Cmin/U
U/A.Cmin
A.U.Cmin
A.U/Cmin
Stanton number
Biot number
Peclet number
Grashoff number