presentation for chapters 5 and 6
DESCRIPTION
Presentation for chapters 5 and 6. LIST OF CONTENTS. Surfaces - Emission and Absorption Surfaces - Reflection Radiative Transfer in the Atmosphere-Ocean System Examples of Phase Functions Rayleigh Phase Function Mie-Debye Phase Function Henyey-Greenstein Phase Function - PowerPoint PPT PresentationTRANSCRIPT
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Presentation for chapters 5 and 6
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LIST OF CONTENTS
1. Surfaces - Emission and Absorption2. Surfaces - Reflection3. Radiative Transfer in the Atmosphere-Ocean System4. Examples of Phase Functions5. Rayleigh Phase Function6. Mie-Debye Phase Function7. Henyey-Greenstein Phase Function8. Scaling Transformations9. Remarks on Scaling Approximations
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SURFACES - EMISSION AND ABSORPTION
• Energy emitted by a surface into whole hemisphere - spectral flux emittance:
• Energy absorped when radiation incident over whole hemisphere – spectral flux absorptance:
• Kirchoff’s Law for Opaque Surface:
Energy emitted relative to that of a blackbody
ss TvTv ,2,,2,
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2. SURFACES - REFLECTION
• Ratio between reflected intensity and incident energy – Bidirectional Reflectance Distribution Function (BRDF):
• Lambert surface – reflected intensity is completely uniform .• Specular surface – reflected intensity in one direction
• In general: BRDF has one specular and one diffuse component:
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SURFACE REFLECTION
Analytic reflectance expressions
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no
kkono
2,
Seeliger-Lommel
yreciprocit of principleobey model This
,
FormulaMinnaert 11
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Transmission through a slab• Transmitance
• Transimitted intensity leaving the medium in downward direction
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TRANSMISSION THROUGH A SLAB
For collimated beam:• Transmitted intensity is
• Flux transmitted
,,coscoscos oo
sv
voo
svvt vFeFI s
dT
dveFF o
vo
svvt
s cos,,cos dT
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TRANSMISSION THROUGH A SLAB
• Flux transmitance is
dve
F
Fv
ov
osv
vto
s cos,,
cos2,,
d
d
T
T
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RADIATIVE TRANSFER EQUATION
direction scattered
directionincident '
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'
vvs
v Ipdva
BaId
dI
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RADIATIVE TRANSFER EQUATION
• For Zero scattering
2
2
1
21 ,,12
solution generalWith
PPtP
P
PP
vvs
v
etdtBePIPI
TBId
dI
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RADIATIVE TRANSFER IN THE ATMOSPHERE-OCEAN SYSTEM
• The refractive index is in the atmosphere and in the ocean.
• In aquatic media, radiative transfer similar to gaseous media• In pure aquatic media Density fluctuations lead to Rayleigh-like
scattering.
• In principle: Snell’s law and Fresnel’s equations describe radiative coupling between the two media if ocean surface is calm.
• Complications are due to multiple scattering and total internal reflection as below
1rm 34.1rm
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RADIATIVE TRANSFER IN THE ATMOSPHERE-OCEAN SYSTEM
• Demarcation between the refractive and the total reflective region in the ocean is given by the critical angle, whose cosine is:
• where
• Beams in region I cannot reach the atmosphere directly• Must be scattered into region II first
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EXAMPLES OF PHASE FUNCTIONS
• We can ignore polarization effects in many applications eg:• Heating/cooling of medium,Photodissociation of molecules’Biological dose
rates
• Because: Error is very small compared to uncertainties determining optical properties of medium.
• Since we are interested in energy transfer-> concentrate on the phase function
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RAYLEIGH PHASE FUNCTION
• Incident wave induces a motion (of bound electrons) which is in phase with the wave ,nucleus provides a ’restoring force’ for electronic motion
• All parts of molecule subjected to same value of E-field and the oscillating charge radiates secondary waves
• Molecule extracts energy from wave and re-radiates in all directions
• For isotropic molecule, unpolarized incidenradiation:
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RAYLEIGH PHASE FUNCTION
• Expanding in terms of incident and scattered angles:
• Azimuthal-averaged phase function is:
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RAYLEIGH PHASE FUNCTION
• By expressing in terms of Legendre Polynomials:
• Asymmetry factor for Rayleigh phase function is zero (because of orthogonality of Legendre Polynomials):
• Only non-zero moment is
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MIE-DEBYE PHASE FUNCTION
• Scattering by spherical particles
• Scattering by larger particles:-> Strong forward scattering – diffraction peak in forward direction!
• Why?• For a scattering object small compared to
wavelength:-> Emission add together coherently because all oscillating dipoles are subject to the same field
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MIE-DEBYE PHASE FUNCTION
• For a scattering object large compared to wavelength:
• All parts of dipole no longer in phase
• We find that:
• Scattered wavelets in forward direction: always in phase
• Scattered wavelets in other directions: mutual cancellations, partial interference
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HENYEY-GREENSTEIN PHASE FUNCTION
• A one-parameter phase function first proposed in 1941:
• No physical basis, but very popular because of the remarkable feature:
• Legendre polynomial coeffients are simply:
• Only first moment of phase function must be specified, thus HG expansion is simply: