k. A. (dT/dx)
k. A. (dx/dT)
k. (dT/dx)
k. (dx/dT)
A. k. A. (dT/dx)
Stanton number
Biot number
Peclet number
Grashoff number
Is black in colour
Reflects all heat
Transmits all heat radiations
Absorbs heat radiations of all wave lengths falling on it
Reflected
Refracted
Transmitted
Absorbed
Better insulation should be put over pipe and better one over it
Inferior insulation should be put over pipe and better one over it
Both may be put in any order
Whether to put inferior OIL over pipe or the better one would depend on steam temperature
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.
Reynold's number
Grashoff's number
Reynold's number, Grashoff's number
Prandtl number, Grashoff's number
First law of thermodynamics
Newton's law of cooling
Newton's law of heating
Stefan's law
k. A. (dT/dx)
k. A. (dx/dT)
k. (dT/dx)
k. (dx/dT)
Parallel flow
Counter flow
Cross flow
All of these
Increases
Decreases
Remain constant
May increase or decrease depending on temperature
Watt/cm² °K
Watt/cm4 °K
Watt²/cm °K⁴
Watt/cm² °K⁴
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
h = k/ ρS
h = ρS/k
h = S/ρk
h = kρ/S
Free electrons
Atoms colliding frequency
Low density
Porous body
Higher
Lower
Same
Depends on the area of heat exchanger
Directly proportional to the thermal conductivity
Inversely proportional to density of substance
Inversely proportional to specific heat
All of the above
Kirchhoff's law
Stefan's law
Wines law
Planck's law
Fourier equation
Stefan-Boltzmann equation
Newton Reichmann equation
Joseph-Stefan equation
Equal to one
Greater than one
Less than one
Equal to Nusselt number
Same
More
Less
Depends on other factors
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
Conduction
Convection
Radiation
Conduction and convection
Different heat contents
Different specific heat
Different atomic structure
Different temperatures
I.C. engine
Air preheaters
Heating of building in winter
None of the above
Convection
Radiation
Conduction
Both convection and conduction
Pb = pa - pv
Pb = pa + pv
Pb = pa × pv
Pb = pa/pv
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
Increases
Decreases
Remain constant
May increase or decrease depending on temperature
Absolute temperature
Square of the absolute temperature
Cube of the absolute temperature
Fourth power of the absolute temperature
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