Reynold's number
Grashoff's number
Reynold's number, Grashoff's number
Prandtl number, Grashoff's number
D. Prandtl number, Grashoff's number
1 : 1
2 : 1
1 : 2
4 : 1
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.
Cold body to hot body
Hot body to cold body
Smaller body to larger body
Larger body to smaller body
tm = (Δt1 - Δt2)/ loge (Δt1/Δt2)
tm = loge (Δt1/Δt2)/ (Δt1 - Δt2)
tm = tm = (Δt1 - Δt2) loge (Δt1/Δt2)
tm = loge (Δt1 - Δt2)/ Δt1/Δt2
Stanton number
Biot number
Peclet number
Grashoff number
Grashoff number and Reynold number
Grashoff number and Prandtl number
Prandtl number and Reynold number
Grashoff number, Prandtl number and Reynold number
J/m² sec
J/m °K sec
W/m °K
Option (B) and (C) above
S.H/(S.H + L.H)
(S.H + L.H) /S.H
(L.H - S.H)/S.H
S.H/(L.H - S.H)
Melting of ice
Boiler furnaces
Condensation of steam in condenser
None of these
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
Free convection
Forced convection
Radiation
Electric heater
Steam condenser
Boiler
Refrigerator condenser coils
Parallel flow
Counter flow
Cross flow
All of these
Same
Higher
More or less same
Very much lower
Universal gas constant
Kinematic viscosity
Thermal conductivity
Planck's constant
Black radiation
Full radiation
Total radiation
All of these
Directly proportional to thermal conductivity
Inversely proportional to density of substance
Inversely proportional to specific heat
All of the above
P = 0, x = 0 and a = 1
P=1, T = 0 and a = 0
P = 0, x = 1 and a = 0
X = 0, a + p = 1 Where a = absorptivity, p = reflectivity, x = transmissivity
0
0.5
0.75
1
Conduction
Free convection
Forced convection
Radiation
Varies with temperature
Varies with the wave length of incident ray
Varies with both
Does not vary with temperature and wave length of the incident ray
W/m²K
W/m²
W/mK
W/m
Solids
Liquids
Gases
None of these
Move actually
Do not move actually
Affect the intervening medium
Does not affect the intervening medium
At all temperatures
At one particular temperature
When system is under thermal equilibrium
At critical temperature
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
Quantity of heat flowing in one second through one cm cube of material when opposite faces ^re maintained at a temperature difference of 1°C
Quantity of heat flowing in one second through a slab of the material of area one cm square, thickness 1 cm when its faces differ in temperature by 1°C
Heat conducted in unit time across unit area through unit thickness when a temperature difference of unity is maintained between opposite faces
All of the above
Free electrons
Atoms colliding frequency
Low density
Porous body
Increases
Decreases
Remain constant
May increase or decrease depending on temperature
A.Cmin/U
U/A.Cmin
A.U.Cmin
A.U/Cmin