Stanton number
Biot number
Peclet number
Grashoff number
A. Stanton number
Is black in colour
Reflects all heat
Transmits all heat radiations
Absorbs heat radiations of all wave lengths falling on it
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
k₁ k₂
(k₁ + k₂)
(k₁ + k₂)/ k₁ k₂
2 k₁ k₂/ (k₁ + k₂)
Black radiation
Full radiation
Total radiation
All of these
Their atoms collide frequently
Their atoms are relatively far apart
They contain free electrons
They have high density
Absolute temperature
Square of temperature
Fourth power of absolute temperature
Fourth power of temperature
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
Thermal conductivity
Thermal diffusivity
Density
Dynamic viscosity
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
Universal gas constant
Kinematic viscosity
Thermal conductivity
Planck's constant
Grey body
Brilliant white polished body
Red hot body
Black body
One
Two
Three
Four
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.
Cold water inlet and outlet
Hot medium inlet and outlet
Hot medium outlet and cold water inlet
Hot medium outlet and cold water outlet
Absolute temperature (T)
I²
F
T
0.45
0.55
0.40
0.75
Conduction
Convection
Radiation
Conduction and radiation combined
Hr (time)
Sq. m (area)
°C (temperature)
K.cal (heat)
More than those for liquids
Less than those for liquids
More than those for solids
Dependent on the viscosity
h₁ + h₂ + h₃
(h₁.h₂.h₃)1/3
1/h₁ + 1/h₂ + 1/h₃
None of these
Conduction
Convection
Radiation
Scattering
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.
A dimensionless parameter
Function of temperature
Used as mathematical model
A physical property of the material
Conduction
Convection
Radiation
Conduction and convection
Density
Coefficient of viscosity
Gravitational force
All of these
Increases
Decreases
Remain constant
May increase or decrease depending on temperature
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
Increases
Decreases
Remain constant
May increase or decrease depending on temperature
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)
Equal to one
Greater than one
Less than one
Equal to Nusselt number