FEA Based Level 3 Assessment of Deformed Tanks with Fluid Induced Loads
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Radiation
1. TITLE : RADIATIONS, BASIC CONCEPT OF
RADIATION , STEFAN BOLTZMANN LAW.
๏ต SHIVAM PATEL 150110105031
๏ต VATSAL PATEL 150110105032
๏ต VYOM PATODIYA 150110105033
๏ต KRISHNA PESHIVADIYA 150110105034
DEPARTMENT OF CHEMICAL ENGINEERING
G H PATEL COLLEGE OF ENGINEERING AND TECHNOLOGY
VALLABHVIDYA NAGAR- 388120
SUBJECT : PROCESS HEAT TRANSFER
2. OVERVIEW :-
๏ต WHAT IS RADIATION
๏ต CHARECTERISTIC OF RADIATION
๏ต BASIC CONCEPT OF RADIATION
๏ต THE STEFAN-BOLTZMANN LAW
3. WHAT IS RADIATION??
๏ต RADIATION is the emission or transmission of
energy in the form of waves or particles through
space or through a material medium.
๏ต Heat transfer through an evacuated can occur
only by radiation.
4. Characteristic of radiation:
๏ต The electromagnetic waves are emitted as a result of vibrational
and rotational movement of molecular of the matter.
๏ต The general phenomenon of radiation covers all wavelength from
shorter to longer.
๏ต The frequency of wavelength is related by
C=ฮปฯ
5. ๏ต Radiation can be reflected an absorption when the pass
through a media.
๏ต All matter emits radiant energy and body at high
temperature emits at greater rate than low temperature.
๏ต Heat exchange by radiation gets enhanced at elevated
temperature of the source and the surrounding.
6. BASIC CONCEPTS OF RADIATION FROM A
SURFACE
๏ต Thermal radiation incident on a body tends to increase its temperature. Its
depend on the nature of material and its surface characteristic.
๏ต The light falling on a body the small part of light is reflecting and mostly
absorbed.
๏ต Absorption, reflection and transmission of incident radiation.
7. ๏ต Another important property of the surface of the
substance is its ability to emit radiation .
๏ต Emission of radiation should not be confused with
reflection.
๏ต Reflection may occur only when a surface receives
radiation, emission of radiation always occurs if the
temperature of the surface is above absolute zero.
๏ต Reflection and emission of radiation depend upon the
surface characteristics.
๏ต Emissivity of a surface is a measure of how good it is an
emitter.
8. ๏ต BLACK BODY:
๏ต Its effective absorbers of radiation in the wavelength that are
encountered in heat transfer
๏ต According to name black body is perfect absorber of radiation.
๏ต ฮฑ =1 , ฯ=ฯ=0
๏ต GREAY BODY:
๏ต When a body absorbed a certain fixed percentages of radiations surface is called the
gray body.
๏ต WHITE BODY:
๏ต A body which is reflect all the accident thermal radiation is called white
body.
๏ต It is known a specular body.
๏ต ฮก=1 , ฮฑ=ฯ=0.
9. THE STEFAN BOLTZMANN LAW
๏ต StefanโBoltzmann law, statement that the total radiant
heat energy emitted from a surface is proportional to the
fourth power of its absolute temperature.
๏ต Determine the total emissive power of a black body by
Stefan Boltzmann law.
10.
11. ๏ต Above equation is known as Stefan Boltzmann equation.
๏ต Which allow us to calculate the total amount of wavelength
emitted in all possible directions by a black body.
๏ต The value of Stefan Boltzmann constant ๐ has been determined
experimentally by a number of researchers.
๏ต The accepted experimentally value is
๐=5.67*10
๏ The unit of Stefan Boltzmann constant is W/๐ ๐ ๐ฒ ๐.
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