One
Two
Three
Four
C. Three
Varies with temperature
Varies with wavelength of the incident ray
Is equal to its emissivity
Does not vary with temperature and. wavelength of the incident ray
Glass
Water
Plastic
Air
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
Composition
Density
Porosity
All of the above
K cal/kg m² °C
K cal m/hr m² °C
K cal/hr m² °C
K calm/hr °C
Liquids
Energy
Temperature
Entropy
Absolute temperature (T)
I²
F
T
1 : 1
2 : 1
1 : 2
4 : 1
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
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.
High thickness of insulation
High vapour pressure
Less thermal conductivity insulator
A vapour seal
S.H/(S.H + L.H)
(S.H + L.H) /S.H
(L.H - S.H)/S.H
S.H/(L.H - S.H)
Watt/mK
Watt/m²K²
Watt/m²K4
Watt/mK²
k/h₀
2k/h₀
h₀/k
h₀/2k
Hr (time)
Sq. m (area)
°C (temperature)
K.cal (heat)
W/m²K
W/m²
W/mK
W/m
k₁ k₂
(k₁ + k₂)
(k₁ + k₂)/ k₁ k₂
2 k₁ k₂/ (k₁ + k₂)
Aluminium
Steel
Brass
Copper
Radiators in automobile
Condensers and boilers in steam plants
Condensers and evaporators in refrigeration and air conditioning units
All of the above
Kirchhoff's law
Stefan's law
Wines law
Planck's law
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.
Solids
Liquids
Gases
None of these
Same
Higher
More or less same
Very much lower
Grashoff number
Biot number
Stanton number
Prandtl number
P = 0, x = 0 and a = 1
P=1, x = 0 and a = 0
P = 0, x = 1 and a = 0
X = 0, a + p = 1 Where a = absorptivity, p = reflectivity, X = transmissivity.
Free electrons
Atoms colliding frequency
Low density
Porous body
First law of thermodynamics
Newton's law of cooling
Newton's law of heating
Stefan's law
α = 1, ρ = 0 and τ = 0
α = 0, ρ = 1 and τ = 0
α = 0, ρ = 0 and τ = 1
α + ρ = 1 and τ = 0
Conduction
Convection
Radiation
Conduction and convection
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