An optical pyrometer calibrated for an ideal black body radiation gives too low a value for temperature of a red-hot iron piece kept in the open. Black body radiation equation is given byE=σ(T4−T40)
this equation is also known as Stefan's law of radiation .
Where,
E = Energy radiation
T = Temperature of optical pyrometer
T0= Temperature of open space
σ = Stefan's constant
from
above formula, it is clearly shown that, an increase in the temperature of open
space reduces the radiation energy. When the same piece of iron is placed in a
furnace, the radiation energy, E=σT4