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
B. P=1, T = 0 and a = 0
Grashoff number
Nusselt number
Weber number
Prandtl number
Increases
Decreases
Remain constant
May increase or decrease depending on temperature
m²/hr
m²/hr °C
kcal/m² hr
kcal/m. hr °C
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
h₁ + h₂ + h₃
(h₁.h₂.h₃)1/3
1/h₁ + 1/h₂ + 1/h₃
None of these
Conduction
Convection
Radiation
None of these
Solids
Liquids
Gases
None of these
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
Hr (time)
Sq. m (area)
°C (temperature)
K.cal (heat)
Black radiation
Full radiation
Total radiation
All of these
Velocity reduction method
Equal friction method
Static regains method
Dual or double method
A dimensionless parameter
Function of temperature
Used as mathematical model
A physical property of the material
Convection
Radiation
Forced convection
Free convection
RN = hl/k
RN = μ cp/k
RN = ρ V l /μ
RN = V²/t.cp
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
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
Grashoff number and Reynold number
Grashoff number and Prandtl number
Prandtl number and Reynold number
Grashoff number, Prandtl number and Reynold number
Watt/mK
Watt/m²K²
Watt/m²K4
Watt/mK²
Conduction
Convection
Radiation
Conduction and radiation combined
Conduction
Convection
Radiation
None of these
Wien's law
Stefan's law
Kirchhoff's law
Planck's law
At all temperatures
At one particular temperature
When system is under thermal equilibrium
At critical temperature
Increases
Decreases
Remain constant
May increase or decrease depending on temperature
Irregular surfaces
Nonuniform temperature surfaces
One dimensional cases only
Two dimensional cases only
Same
Less
Greater
None of these
Higher
Lower
Same
Depends on the area of heat exchanger
Grey body
Brilliant white polished body
Red hot body
Black body
Thermometer
Thermistor
Thermocouple
None of these
k. A. (dT/dx)
k. A. (dx/dT)
k. (dT/dx)
k. (dx/dT)
Stanton number
Biot number
Peclet number
Grashoff number