RN = hl/k
RN = μ cp/k
RN = ρ V l /μ
RN = V²/t.cp
C. RN = ρ V l /μ
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
RN = hl/k
RN = μ cp/k
RN = ρ V l /μ
RN = V²/t.cp
2 TR
4 TR
8 TR
10 TR
Conduction
Convection
Radiation
None of these
In conduction, reduction in the thickness of the material and an increase in thermal conductivity.
In convection, stirring of the fluid and cleaning the heating surface.
In radiation, increasing the temperature and reducing the emissivity.
All of the above
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.
Free electrons
Atoms colliding frequency
Low density
Porous body
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
Zeroth law of thermodynamics
First law of thermodynamics
Second law of thermodynamics
Kirchhoff's law
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
1 : 1
2 : 1
1 : 2
4 : 1
Reflected
Refracted
Transmitted
Absorbed
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)
Black bodies
Polished bodies
All coloured bodies
All of the above
Black body
Grey body
Opaque body
White body
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
Conduction
Convection
Radiation
Conduction and convection
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.
Equal to one
Greater than one
Less than one
Equal to Nusselt number
Pb = pa - pv
Pb = pa + pv
Pb = pa × pv
Pb = pa/pv
Wien's law
Stefan's law
Kirchhoff's law
Planck's law
Conduction
Convection
Radiation
Conduction and convection
Fourier equation
Stefan-Boltzmann equation
Newton Reichmann equation
Joseph-Stefan equation
Temperature
Thickness
Area
Time
Melting of ice
Boiler furnaces
Condensation of steam in condenser
None of these
k₁ k₂
(k₁ + k₂)
(k₁ + k₂)/ k₁ k₂
2 k₁ k₂/ (k₁ + k₂)
Temperature
Wave length
Physical nature
All of the above
k/h₀
2k/h₀
h₀/k
h₀/2k
Thermal conductivity to the equivalent thickness of the film of fluid
Temperature drop through the films of fluids to the thickness of film of fluids
Thickness of film of fluid to the thermal conductivity
Thickness of film of fluid to the temperature drop through the films of fluids
Blast furnace
Heating of building
Cooling of parts in furnace
Heat received by a person from fireplace