unit two thermal radiationfac.ksu.edu.sa/sites/default/files/unit_2_-_thermal_radiation_2.pdf · 4...
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ME 476
Solar Energy
UNIT TWO
THERMAL RADIATION
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Unit Outline
• Electromagnetic radiation
• Thermal radiation
• Blackbody radiation
• Radiation emitted from a real surface
• Irradiance
• Kirchhoff’s Law
• Diffuse and gray surface
• View factor
• Radiation exchange between black bodies
• Radiation from a diffuse, gray surface
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Electromagnetic Radiation
• The electromagnetic energy emitted by matter as a result
of the changes in the electronic configurations of the
atoms or molecules.
• Electromagnetic radiation energy is transported by waves
• These waves have a frequency () and wavelength ().
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• Frequency and wavelength Are related by:
where,
C = C0 / n
C: the speed of propagation of a wave in the medium
C0 = 2.9979108 m/s, the speed of light in a vacuum
n, the index of refraction of that medium
Examples:
n =1 (air and most gases)
n = 1.5 (glass)
n = 1.33 (water)
Electromagnetic Radiation
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• Radiation differs from conduction and convection
• It does not require the presence of a material medium
• Radiation transfer occurs in all types of matter (solid,
liquid, or gas)
Electromagnetic Radiation
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• Electromagnetic radiation can be viewed as the
propagation of a collection of discrete packets of energy
called photons or quanta.
• In this view, each photon of frequency (n) is considered to
have an energy of:
where h is called Planck’s constant
h = 6.6256 x 10-34 J.s
• This means that the energy of a photon is inversely
proportional to its wavelength
Electromagnetic Radiation
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Unit Outline
• Electromagnetic radiation
• Thermal radiation
• Blackbody radiation
• Radiation emitted from a real surface
• Irradiance
• Kirchhoff’s Law
• Diffuse and gray surface
• View factor
• Radiation exchange between black bodies
• Radiation from a diffuse, gray surface
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Thermal Radiation
• Thermal radiation is the part of electromagnetic radiation
that primarily creates a heating effect.
• Thermal radiation is emitted as a result of energy
transitions of molecules, atoms, and electrons of a
substance.
• Temperature is a measure of the strength of these
activities at the microscopic level
• Therefore, thermal radiation emission increases with
increasing temperature
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• Thermal radiation mainly covers:
• Infrared radiation
• Visible light
• Ultraviolet radiation
Thermal Radiation
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Unit Outline
• Electromagnetic radiation
• Thermal radiation
• Blackbody radiation
• Radiation emitted from a real surface
• Irradiance
• Kirchhoff’s Law
• Diffuse and gray surface
• View factor
• Radiation exchange between black bodies
• Radiation from a diffuse, gray surface
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Blackbody Radiation
• A blackbody is a body that absorbs all the incident
radiation regardless of wavelength and direction AND
emits the maximum amount radiation at a given
temperature.
• It is an idealized body to serve as a standard against
which the radiative properties of real surfaces may be
compared.
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Blackbody Radiation
• The amount of radiation emitted by a blackbody is given
by Planck’s Law:
where,
k = 1.381 x 10-23 J/K (Boltzmann’s Constant)
• Planck’s Law shows that the
energy emitted from a blackbody
does not depend on direction.
• Blackbody radiation is diffuse.
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Blackbody Radiation
• From Planck’s Law, we can find the wavelength at which
the maximum radiation is emitted by a blackbody
• This is done by taking the derivative of E b and setting it
to zero
• The result is called Wien’s displacement law:
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Blackbody Radiation
Locus of
maximum power
T = 2897.8 mm.K
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Blackbody Radiation
• Integrating Planck’s Law yields Stefan-Boltzmann’s
Equation:
where,
s = 5.67 x 10-8 W/m2.K4 (Stefan-Boltzmann Constant)
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Unit Outline
• Electromagnetic radiation
• Thermal radiation
• Blackbody radiation
• Radiation emitted from a real surface
• Irradiance
• Kirchhoff’s Law
• Diffuse and gray surface
• View factor
• Radiation exchange between black bodies
• Radiation from a diffuse, gray surface
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Radiation Emitted from a Real Surface
• A real surface does not emit as much energy as a blackbody.
• A real surface does not emit energy uniformly in all directions.
• The amount of energy emitted by a real surface is quantified
by emittance.
• Emittance is the ratio of radiation emitted by a real surface to
the radiation emitted by a blackbody at the same temperature.
• When the energy emitted in all directions and at all
wavelengths is integrated, the result is the “total
hemispherical emittance”
• Emittance ranges from 0 to 1.
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Unit Outline
• Electromagnetic radiation
• Thermal radiation
• Blackbody radiation
• Radiation emitted from a real surface
• Irradiance
• Kirchhoff’s Law
• Diffuse and gray surface
• View factor
• Radiation exchange between black bodies
• Radiation from a diffuse, gray surface
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Irradiance
• Irradiance is the rate at which radiant energy is incident
on a surface per unit area of that surface (W/m2).
• Some references refer to irradiance as “incident radiation”
• It is usually denoted with (G).
• Irradiance can be either:
• Absorbed
• Reflected
• Transmitted (if the medium is transparent)
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Irradiance
• The ratio of absorbed irradiance
to total irradiance is called
absorptance (a)
• The ratio of reflected irradiance
to total irradiance is called
reflectance (r)
• The ratio of transmitted
irradiance to total irradiance is
called transmittance (t )
Irradiance
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Irradiance
• Absorptance: 𝛼 =Absorbed radiation
Irradiance=
𝐺abs
𝐺, 0 ≤ 𝛼 ≤ 1
• Reflectance: 𝜌 =Reflected radiation
Irradiance=
𝐺ref
𝐺, 0 ≤ 𝜌 ≤ 1
• Transmittance: 𝜏 =Transmitted radiation
Irradiance=
𝐺tr
𝐺, 0 ≤ 𝜏 ≤ 1
• Gabs + Gref + Gtr = G
• a + r + t = 1
• a + r = 1 (for opaque surfaces)
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Unit Outline
• Electromagnetic radiation
• Thermal radiation
• Blackbody radiation
• Radiation emitted from a real surface
• Irradiance
• Kirchhoff’s Law
• Diffuse and gray surface
• View factor
• Radiation exchange between black bodies
• Radiation from a diffuse, gray surface
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Kirchhoff’s Law
The total hemispherical emittance of a surface at
temperature T is equal to its total hemispherical
absorptance for radiation coming from a blackbody at the
same temperature.
• e(T) = a(T)
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Unit Outline
• Electromagnetic radiation
• Thermal radiation
• Blackbody radiation
• Radiation emitted from a real surface
• Irradiance
• Kirchhoff’s Law
• Diffuse and gray surface
• View factor
• Radiation exchange between black bodies
• Radiation from a diffuse, gray surface
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Diffuse and Gray Surface
• A gray surface is a surface whose e and a are
independent of wavelength.
• If the surface is diffuse and gray:
e = a
• In this case, the source of irradiation does not have to
be a blackbody and the source’s temperature does not
have to be equal to the surface temperature
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Unit Outline
• Electromagnetic radiation
• Thermal radiation
• Blackbody radiation
• Radiation emitted from a real surface
• Irradiance
• Kirchhoff’s Law
• Diffuse and gray surface
• View factor
• Radiation exchange between black bodies
• Radiation from a diffuse, gray surface
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View Factor
• The view factor (Fij) is the fraction of the radiation
leaving surface i that strikes surface j directly
• The view factor ranges between 0 and 1.
Fij
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View Factor
EXAMPLE
• The view factor F12 = 1 since all the
radiation leaving Surface 1 hits
Surface 2.
• F21 < 1, since not all the radiation
leaving Surface 2 will hit Surface 1.
• Some of the radiation leaving one
part of Surface 2 will hit another part
on Surface 2 itself.
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View Factor
View factor between two aligned parallel
rectangles of equal size
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View Factor
View factor between two coaxial parallel disks
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View Factor
View factors for two concentric cylinders of finite length
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View Factor Relations
The Reciprocity Relation
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View Factor Relations
The Summation Rule
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Unit Outline
• Electromagnetic radiation
• Thermal radiation
• Blackbody radiation
• Radiation emitted from a real surface
• Irradiance
• Kirchhoff’s Law
• Diffuse and gray surface
• View factor
• Radiation exchange between black bodies
• Radiation from a diffuse, gray surface
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Radiation Exchange Between Two Black Bodies
• If Surface 1 and Surface 2 are blackbodies, the net
radiation heat transfer from Surface 1 to Surface 2 is:
• The reciprocity relation asserts that: A1 F1→2 = A2 F2 → 1
• Also: Eb = s T 4
• Therefore,
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Unit Outline
• Electromagnetic radiation
• Thermal radiation
• Blackbody radiation
• Radiation emitted from a real surface
• Irradiance
• Kirchhoff’s Law
• Diffuse and gray surface
• View factor
• Radiation exchange between black bodies
• Radiation from a diffuse, gray surface
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Radiosity
• Radiation from a diffuse gray
surface differs from radiation
from a black body in two ways:
• The radiation emitted is e Eb
(instead of Eb)
• The reflected radiation is r G
(instead of 0)
• The total radiation energy
leaving a surface per unit time
and per unit area is called
radiosity (J).
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Radiosity
𝐽𝑖 = 𝜀𝑖 𝐸𝑏 + 𝜌𝑖 𝐺𝑖
• But ri + ai = 1
• For a diffuse gray surface, ai = ei
• Therefore: ri + ei = 1
→ ri = 1 – ei
𝐽𝑖 = 𝜀𝑖 𝐸𝑏 + 1 − 𝜀𝑖 𝐺𝑖
𝐺𝑖 =𝐽𝑖 − 𝜀𝑖 𝐸𝑏
1 − 𝜀𝑖
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Net Rate of Radiation Heat Transfer from a Diffuse
Gray Surface
= 𝐴𝑖 𝐽𝑖−𝐺𝑖
=𝐴𝑖 𝜀𝑖
1 − 𝜀𝑖𝐸𝑏𝑖 − 𝐽𝑖
= 𝐴𝑖 𝐽𝑖−𝐽𝑖 − 𝜀𝑖𝐸𝑏
1 − 𝜀𝑖
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Radiation Heat Transfer in Two-Surface Enclosures
• This is true for any two diffuse gray
surfaces.
Example: Radiation from a horizontal
solar collector to the sky at night
• The sky can be considered a
blackbody at a temperature below
ambient