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
C. All bodies above absolute zero emit radiation
Parallel flow type
Counter flow type
Cross flow type
Regenerator type
Less than those for gases
Less than those for liquids
More than those for liquids and gases
More or less same as for liquids and gases
Increases
Decreases
Remain constant
May increase or decrease depending on temperature
Conduction
Convection
Radiation
None of these
Velocity reduction method
Equal friction method
Static regains method
Dual or double method
Conduction
Convection
Radiation
Conduction and convection
Thermal resistance
Thermal coefficient
Temperature gradient
Thermal conductivity
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
I.C. engine
Air preheaters
Heating of building in winter
None of the above
Improve heat transfer
Provide support for tubes
Prevent stagnation of shell side fluid
All of these
Temperature
Thickness
Area
Time
0.45
0.55
0.40
0.75
Equal to
Directly proportional to
Inversely proportional to
None of these
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
Emissivity
Transmissivity
Reflectivity
Intensity of radiation
Conduction
Convection
Radiation
None of these
At all temperatures
At one particular temperature
When system is under thermal equilibrium
At critical temperature
Density
Coefficient of viscosity
Gravitational force
All of these
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
Equal to one
Greater than one
Less than one
Equal to Nusselt number
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
Its temperature
Nature of the body
Kind and extent of its surface
All of the above
-1/3
-2/3
1
-1
From one particle of the body to another without the actual motion of the particles
From one particle of the body to another by the actual motion of the heated particles
From a hot body to a cold body, in a straight line, without affecting the intervening medium
None of the above
Increases
Decreases
Remain constant
May increase or decrease depending on temperature
Grey body
Brilliant white polished body
Red hot body
Black body
Absolute temperature
Square of the absolute temperature
Cube of the absolute temperature
Fourth power of the absolute temperature
0
0.5
0.75
1
Their atoms collide frequently
Their atoms are relatively far apart
They contain free electrons
They have high density
Conduction
Convection
Radiation
Conduction and radiation combined