8/4/2019 Black Body Radiations
1/25
RADIATION PYROMETERS
8/4/2019 Black Body Radiations
2/25
WHY RADIATION PYROMETERS
ARE USED?
Radiation pyrometer
measures the temperature without any physical contact
between the object whose temperature is to be measured andthe sensor
Used for measuring very high temperatures (even above the
range of thermocouples)
Used to measure the temperature ofmoving objects
8/4/2019 Black Body Radiations
3/25
THEORY
Radiation pyrometers measures the thermal radiationsemitted by an object whose temperature is to measured
Thermal radiations are the electromagnetic radiations
emitted as a result oftemperature
The amount of radiations emitted by the object depends on itstemperature
Thermal radiations lies in the wavelength region from 0.1 to100 micro-metres
8/4/2019 Black Body Radiations
4/25
BLACK BODY CONDITIONS
The operation of Radiation Pyrometers are based on black
body concepts
A black body is an object that absorbs 100% of the
radiations that hits it.
A block body reflects no radiations
At a particular temperature, a black body emits maximum
amount of radiations possible for that temperature
8/4/2019 Black Body Radiations
5/25
BLACK BODY CONDITIONS
Thus a black body emits and absorbs maximum amount of
radiations at all the wavelengths
The total thermal radiations emitted by a black body is
in
=Stefan Boltzmann constant=
T=absolute temperature in K
8/4/2019 Black Body Radiations
6/25
CONTINUED
A black body radiates more heat than a smooth bright surface.
We define a term Emissivity,
Where q is the heat radiated by a gray (brighter surface) body
and is the heat radiated by a black body
=1 for a black body and for a gray body, lies in the
range of 0 to1
8/4/2019 Black Body Radiations
7/25
CONTINUED
The energy is distributed over a wide range of frequencies in
the electromagnetic spectrum
For any particular wavelength , the thermal radiations aregiven by:
Where C1 and C2 are constants
8/4/2019 Black Body Radiations
8/25
BLACK BODY RADIATION
CURVES
8/4/2019 Black Body Radiations
9/25
RADIATION CURVES
The radiation curves shows emittedpower per unit area as a
function of wavelengths for black bodies at temperature
from 300K to 6000K
Energy radiated at a particular temperature is given by the area
in the band under that temperature curve
As wavelengths increases, radiations intensity increases from0, reaches to a peak value and then again decreases to 0
8/4/2019 Black Body Radiations
10/25
CONTINUED
With the increase in temperature
Emitted power per unit area increases
Peak(maximum) wavelength emitted by a black bodydecreases
(So, the peak wavelength moves from the infra-red to the visible
region of the spectrum)
Peak wavelength is given by; T is absolute temp in K
8/4/2019 Black Body Radiations
11/25
OPTICAL PYROMETERS
Also called as disappearing filament pyrometers and
monochromatic-brightness radiation thermometers
Most accurate radiation thermometers for temperatures above
than 700
PRINCIPLE: The radiation intensity and the color of thesurface(brightness) varies with temperature
8/4/2019 Black Body Radiations
12/25
DISAPPEARING FILAMENT OPTICAL PYROMETER
8/4/2019 Black Body Radiations
13/25
CONSTRUCTION
An eye piece at one end and an objective lens at the other end.
A power source (battery), rheostat and ammeter (to measure
current) connected to a reference temperature lamp
An absorption screen is placed in between the objective lens
and reference temperature lamp (used to increase the range of
the temperature which can be measured by the instrument)
Red filter between the eye piece and the lamp allows only a
narrow band of wavelengths around .655
8/4/2019 Black Body Radiations
14/25
(A) FILAMENT TOO DARK
(B) FILAMENT TOO BRIGHT (C) EQUAL BRIGHTNESS
8/4/2019 Black Body Radiations
15/25
WORKING
Radiations from the temperature source is focused on a
filament of the lamp using an objective lens
Eye piece is also adjusted until the filament of the lamp isproperly viewed
Filament of the lamp is superimposed on the image of the
target source
8/4/2019 Black Body Radiations
16/25
WORKING CONTINUED
BY CONTROLLING THE LAMP CURRENT, IT WILL BESEEN THAT
(A)the filament will appear dark as if the filament is cooler than
the temperature source
(B) the filament will appear bright as if the filament is hotterthan the temperature source
(C)the filament will not be seen if the filament andtemperature source are in the same temperature
8/4/2019 Black Body Radiations
17/25
CONTINUED
The current through the lamp filament should be adjusted
until the filament and the image are ofequal brightness
The current flowing through the lamp is measured by theammeter which is an indication of the temperature of the
source when calibrated
8/4/2019 Black Body Radiations
18/25
FORMULAE
If the target is not a black body (Emissivity
8/4/2019 Black Body Radiations
19/25
ADVANTAGES
Physical contact of the instrument is not required to
measure temperature of the temperature source.
Accuracy is high
Provided a proper sized image of the temperature sourceis obtained in the instrument, the distance between the
instrument and the temperature source does not matter
Easy to operate
8/4/2019 Black Body Radiations
20/25
DISADAVANTAGES
Since it is manually operated, it cannot be used for the
continuous monitoring and controlling purpose
8/4/2019 Black Body Radiations
21/25
APPLICATIONS
Used to measure temperature of molten metals or heated
materials.
Used to measure temperature of furnace and hot bodies
8/4/2019 Black Body Radiations
22/25
PHOTON DETECTORS
Photon detectors are the infrared detectors that detects the
radiations form any object
Radiations from the object when focused on the photondetector in turn produces an electric output directly related to
the received radiant energy
Base on semiconductor materials
Facilitates temperature measurement from a distance without
contact with the object to be measured.
8/4/2019 Black Body Radiations
23/25
CONTINUED
When the material is exposed to radiations, the individual
photons may add enough energy to some of the electrons such
that they can cross the forbidden energy gap
Eg: Photodiodes
Photons carry an energy E (eV) related to wavelength ( ) as
8/4/2019 Black Body Radiations
24/25
CONTINUED
For antimonide (InSb) , Band gap energy= .22eV
This material will not be sensitive to the wavelength greater
than about 5.6 (its cut off wavelenth)
Photons with wavelength greater than cut off wavelength will
pass through the material undetected
8/4/2019 Black Body Radiations
25/25
INFRARED PYROMETERS
FIELD OF VIEW OF AN INFRARED PYROMETER
The field of view is the angle of vision at which the instrument operates
The object whose temperature is to be measured must fill the field of view of the
instruments