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:-
DEFINITION OF RADIATION
SPECTRUM OF ELECTROMAGNETIC REDIATIONS.
SURFACE EMISSION PROPERTIES.
ABSORPTIVITY, REFLECTIVITY AND TRANSMISSIVITY
BLACK BODY
OPAQUE BODY
WHITE BODY
GRAY BODY
The transfer of energy across a system boundary
by means of an electromagnetic mechanism wich
is caused solely by a temperature difference.
Radiation heat transfer does not require a
medium.
The radiant heat exchange between two bodies
depends on the difference between their
temperature to the Fourth power.
E=σT4 W/m2
E=σAT4 watt
The electromagnetic (EM) spectrum is the range of all types of EM radiation. Radiation is energy that
travels and spreads out as it goes – the visible light that comes from a lamp in your house and the radio
waves that come from a radio station are two types of electromagnetic radiation. The other types of EM
radiation that make up the electromagnetic spectrum are microwaves, infrared light, ultraviolet light, X-
rays and gamma-rays.
Radio: Your radio captures radio waves emitted by radio stations, bringing
your favorite tunes. Radio waves are also emitted by stars and gases in
space.
Microwave: Microwave radiation will cook your popcorn in just a few
minutes, but is also used by astronomers to learn about the structure of
nearby galaxies.
Infrared: Night vision goggles pick up the infrared light emitted by our skin
and objects with heat. In space, infrared light helps us map the dust between
stars.
Visible: Our eyes detect visible light. Fireflies, light bulbs, and stars all emit
visible light.
Ultraviolet: Ultraviolet radiation is emitted by the Sun and are the reason
skin tans and burns. "Hot" objects in space emit UV radiation as well.
X-ray: A dentist uses X-rays to image your teeth, and airport security uses
them to see through your bag. Hot gases in the Universe also emit X-rays.
Gamma ray: Doctors use gamma-ray imaging to see inside your body. The
biggest gamma-ray generator of all is the Universe.
The rate of emission of radiation by a body depends upon the following factors:-
A. Temperature of surface.
B. The nature of surface, and
C. the wavelength or frequency of radiation.
The parameters which deals with the surface emission propertiesare given below:-
1. Total emissive power:-Total amount of radiation emitted by a body per unit area and time.
Eb=σT4 W/m2
Eb=σAT4 watt σ=Stefan-Boltzmann Constant=5.67x10-8 w/m2K4
2. Monochromatic emissive power:- The rate of energy radiated per unit area of the surface
per unit wavelength.
3. Emission from real surface emissivity:- It can be calculated by.
Eb=ἐσAT4
ἐ=Emissivity of the material=Ability of the surface of a body to radiate heat.
Let,
G=Incident radiation
Gr=Reflected radiation
Gt=Transmitted radiation
Ga=Absorbed radiation
By the conservation of energy principle
Ga +Gt +Gr =G
Dividing both sides by G, We get
ABSORBED RADIATIONS
Blackbody is an idealized physical body that absorbs all incident
electromagnetic radiation, regardless of frequency or angle of
incidence.
For a black body, τ = 0, α = 1, and ρ = 0.
Planck offers a theoretical model for perfectly black bodies,
which he noted do not exist in nature: besides their opaque interior,
They have interfaces that are perfectly transmitting and non-reflective.
When no incident radiarions is
transmitted through the body, It is
called an “Opaque Body”
That is, τ = 0 and α + ρ = 1.
ABSORBED RADIATIONS
If all the incident radiation falling
on the body are reflected , It is
called “White Body”.
That is, τ = 1 and α = ρ = 0.
Type of reflection
1. Regular reflection
2. diffuse reflection
A grey body is defined as a body
with constant emissivity over all
wavelengths and temperatures.
or
A grey body is one where α, ρ and
τ are constant for all wavelengths.
Radiation and its properties

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Radiation and its properties

  • 1.
  • 2. :- DEFINITION OF RADIATION SPECTRUM OF ELECTROMAGNETIC REDIATIONS. SURFACE EMISSION PROPERTIES. ABSORPTIVITY, REFLECTIVITY AND TRANSMISSIVITY BLACK BODY OPAQUE BODY WHITE BODY GRAY BODY
  • 3. The transfer of energy across a system boundary by means of an electromagnetic mechanism wich is caused solely by a temperature difference. Radiation heat transfer does not require a medium. The radiant heat exchange between two bodies depends on the difference between their temperature to the Fourth power. E=σT4 W/m2 E=σAT4 watt
  • 4. The electromagnetic (EM) spectrum is the range of all types of EM radiation. Radiation is energy that travels and spreads out as it goes – the visible light that comes from a lamp in your house and the radio waves that come from a radio station are two types of electromagnetic radiation. The other types of EM radiation that make up the electromagnetic spectrum are microwaves, infrared light, ultraviolet light, X- rays and gamma-rays. Radio: Your radio captures radio waves emitted by radio stations, bringing your favorite tunes. Radio waves are also emitted by stars and gases in space. Microwave: Microwave radiation will cook your popcorn in just a few minutes, but is also used by astronomers to learn about the structure of nearby galaxies. Infrared: Night vision goggles pick up the infrared light emitted by our skin and objects with heat. In space, infrared light helps us map the dust between stars. Visible: Our eyes detect visible light. Fireflies, light bulbs, and stars all emit visible light. Ultraviolet: Ultraviolet radiation is emitted by the Sun and are the reason skin tans and burns. "Hot" objects in space emit UV radiation as well. X-ray: A dentist uses X-rays to image your teeth, and airport security uses them to see through your bag. Hot gases in the Universe also emit X-rays. Gamma ray: Doctors use gamma-ray imaging to see inside your body. The biggest gamma-ray generator of all is the Universe.
  • 5. The rate of emission of radiation by a body depends upon the following factors:- A. Temperature of surface. B. The nature of surface, and C. the wavelength or frequency of radiation. The parameters which deals with the surface emission propertiesare given below:- 1. Total emissive power:-Total amount of radiation emitted by a body per unit area and time. Eb=σT4 W/m2 Eb=σAT4 watt σ=Stefan-Boltzmann Constant=5.67x10-8 w/m2K4 2. Monochromatic emissive power:- The rate of energy radiated per unit area of the surface per unit wavelength. 3. Emission from real surface emissivity:- It can be calculated by. Eb=ἐσAT4 ἐ=Emissivity of the material=Ability of the surface of a body to radiate heat.
  • 6. Let, G=Incident radiation Gr=Reflected radiation Gt=Transmitted radiation Ga=Absorbed radiation By the conservation of energy principle Ga +Gt +Gr =G Dividing both sides by G, We get ABSORBED RADIATIONS
  • 7. Blackbody is an idealized physical body that absorbs all incident electromagnetic radiation, regardless of frequency or angle of incidence. For a black body, τ = 0, α = 1, and ρ = 0. Planck offers a theoretical model for perfectly black bodies, which he noted do not exist in nature: besides their opaque interior, They have interfaces that are perfectly transmitting and non-reflective.
  • 8. When no incident radiarions is transmitted through the body, It is called an “Opaque Body” That is, τ = 0 and α + ρ = 1. ABSORBED RADIATIONS
  • 9. If all the incident radiation falling on the body are reflected , It is called “White Body”. That is, τ = 1 and α = ρ = 0. Type of reflection 1. Regular reflection 2. diffuse reflection
  • 10. A grey body is defined as a body with constant emissivity over all wavelengths and temperatures. or A grey body is one where α, ρ and τ are constant for all wavelengths.