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.
D. Ratio of emissive power to absorptive power for all bodies is same and is equal to the emissive power of a perfectly black body.
Direct mixing of hot and cold fluids
A complete separation between hot and cold fluids
Flow of hot and cold fluids alternately over a surface
Generation of heat again and again
Conduction
Free convection
Forced convection
Radiation
Directly proportional to the thermal conductivity
Inversely proportional to density of substance
Inversely proportional to specific heat
All of the above
Thermal conductivity
Thermal diffusivity
Density
Dynamic viscosity
More than those for liquids
Less than those for liquids
More than those for solids
Dependent on the viscosity
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)
Parallel flow type
Counter flow type
Cross flow type
Regenerator type
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
Conduction
Convection
Radiation
None of these
Higher
Lower
Same
Depends upon the shape of body
Black radiation
Full radiation
Total radiation
All of these
Conduction
Convection
Radiation
None of these
Zeroth law of thermodynamics
First law of thermodynamic
Second law of the thermodynamics
Kirchoff's law
Liquids
Energy
Temperature
Entropy
Thermal resistance
Thermal coefficient
Temperature gradient
Thermal conductivity
Absolute temperature
T²
T⁵
T
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
Different heat contents
Different specific heat
Different atomic structure
Different temperatures
Grashoff number
Nusselt number
Weber number
Prandtl number
Absolute temperature (T)
I²
F
T
Stanton number
Biot number
Peclet number
Grashoff number
Wien's law
Stefan's law
Kirchhoff's law
Planck's law
A dimensionless parameter
Function of temperature
Used as mathematical model
A physical property of the material
Conduction
Convection
Radiation
Conduction and convection
Stanton number
Nusselt number
Biot number
Peclet number
In heat exchanger design as a safety factor
In case of Newtonian fluids
When a liquid exchanges heat with a gas
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
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.