Black Body Radiation and its Units

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15 Questions

What is the main characteristic of thermal radiation?

Transfers heat without heating the medium

Which statement is true about the properties of thermal radiation?

Travels through empty space with the velocity of light

Why is a perfectly black body called perfect absorber and perfect radiator?

It absorbs all radiation and emits radiations of all possible wavelengths

What type of radiation is thermal radiation in terms of wavelength?

Infrared radiation

According to Kirchhoff's Law, what is the relationship between emissive power and absorptive power for a given wavelength and temperature?

They are equal

What happens to the energy that is not absorbed by the surface in the described scenario?

It is reflected or transmitted

In the equilibrium state, what is the relationship between absorptive power and emissive power?

Absorptive power equals emissive power

What characteristic of the hole 'O' allows it to act as a black body radiator in the scenario described?

It has a blackened concave diaphragm limiting radiation

Which law describes the relation between energy density and wavelength for shorter wavelengths?

Wien's Law

In the context of the text, what happens when e λT ≫ 1?

Equation (1) simplifies to Wien's Law

Which law applies to the relation between energy density and wavelength for longer wavelengths?

Rayleigh-Jean's Law

How is the value of the constant described in the text in CGS units?

5.672x10-5 erg / (cm2K4sec)

What instrument was used to measure the black body's temperature according to the text?

Thermocouple

What happens to the intensity of heat radiation as the wavelength increases?

Increases and then decreases

How is the energy distribution in the radiation spectrum of a black body characterized according to the text?

Not uniformly distributed

Learn about the distribution of energy in a black body spectrum and the units used to measure constant values in CGS and MKS systems. Explore how Lummer and Pringsheim studied the distribution of energy among radiation emitted by a black body at different temperatures.

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