PowerPoint Presentation
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Prof. Brandt-Pearce
Lecture 2
Channel Modeling
Optical Wireless Communications
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Attenuation (Loss)
Absorption
Scattering
Rayleigh scattering (atmospheric gases molecules)
Mie scattering (aerosol particles)
Beam divergence
Pointing Loss
Atmospheric (refractive) turbulence
Scintillation
Beam wander
Background light (Sun)
Channel Effects
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Atmospheric attenuation: loss of part of optical energy when traversing atmosphere
: Transmitted Power
: Received Power
: Path Length
Attenuation is due to absorption and/or scattering
: molecular absorption coefficient
: Aerosol absorption coefficient
: molecular scattering coefficient
: Aerosol scattering coefficient
An aerosol is a suspension of solid or liquid particles in a gaseous medium, with size larger than a molecule.
Attenuation
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Weather conditionVisibility range (m)Loss dB/kmThick fog200 300 Moderate fog 500120Light fog 770 100025Thin fog/heavy rain (25mm/hr)1900 200025Haze/medium rain (12.5mm/hr) 2800 4000010Clear/drizzle (0.25mm/hr)18000 200001Very clear23000 500000.2
Weather conditions and their visibility range values 1
1Free-space optics by Willebrand and Ghuman, 2002
Attenuation
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Signal Attenuation coefficient at = 850 nm.
Thick fog
Clear air
Attenuation
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Attenuation
Low Clouds
Very similar to fog
May accompany rain and snow
Rain
Drop sizes larger than fog and wavelength of light
Extremely heavy rain (cant see through it) can take a link down
Water sheeting on windows
Heavy Snow
May cause ice build-up on windows
Whiteout conditions
Sand Storms
Likely only in desert areas; rare in the urban core
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Absorption: the energy of a photon is taken by gas molecules or particles and is converted to other forms of energies
This takes place when there is an interaction between the propagating photons and molecules (present in the atmosphere) along its path
Primarily due to water vapor and carbon dioxide
Wavelength dependent
This leads to the atmosphere having transparent zones (range of wavelengths with minimal absorptions) referred to as the transmission windows
It is not possible to change the physics of the atmosphere, therefore, wavelengths adopted in FSO systems are basically chosen to coincide with the atmospheric transmission windows
Attenuation due to Absorption
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Attenuation due to Absorption
Atmospheric absorption transmittance at sea level over 1820 m horizontal path1
1Free-space optics by Willebrand and Ghuman, 2002
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Attenuation due to Scattering
Scattering: dispersion of a beam into other direction due to particles in air
This results in angular redistribution of the optical field with and without wavelength dependence
Depends on the radius of the particles
Two type of scattering:
Rayleigh scattering (Molecule): elasticscattering of light by molecules andparticulate mattermuch smaller than the wavelength of the incident light.
Mie Scattering (Aerosol): broad class of scattering of light by spherical particles of any diameter.
Scattering phase function at angle is (=cos )1
1 Zachor, A. S., Aureole radiance field about a source in a scattering-absorbing medium, Applied Optics, (1978).
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Rayleigh Scattering (Molecular)
Elasticscattering of light by molecules andparticulate mattermuch smaller than the wavelength of the incident light.
Rayleigh scattering intensity has a very strong dependence on the size of the particles (it is proportional the sixth power of their diameter).
It is inversely proportional to the fourth power of the wavelength of light: the shorter wavelength in visible white light (violet and blue) are scattered stronger than the longer wavelengths toward the red end of the visible spectrum.
The scattering intensity is generally not strongly dependent on the wavelength, but is sensitive to the particle size.
Responsible for the blue color of the sky during the day
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Rayleigh Scattering
For a single molecule, the scattering phase function at angle is 1
where
is the depolarization parameter
A simplified expression describing the Rayleigh scattering 1
: number of particles per unit volume
: the cross-sectional area of scattering
1 Bucholtzr, A., Rayleigh-scattering calculations for the terrestrial atmosphere, Applied Optics 34 (1995).
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Mie Scattering (Fog. Haze, Rain)
Broad class of scattering of light by spherical particles of any diameter.
The scattering intensity is generally not strongly dependent on the wavelength, but is sensitive to the particle size.
Mie scattering intensity for large particles is proportional to the square of the particle diameter.
Coincides with Rayleigh scattering in the special case where the diameter of the particles is much smaller than the wavelength of the light; in this limit, however, the shape of the particles no longer matters.
The scattering phase function at angle is 1
g: aerosol asymmetry parameter given by the mean cosine of the scattering angle
f: aerosol hemispheric backscatter fraction
1 Zachor, A. S., Aureole radiance field about a source in a scattering-absorbing medium, Applied Optics, (1978).
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Attenuation due to Beam Divergence
One of the main advantages of FSO systems is the ability to transmit a very narrow optical beam, thus offering enhanced security But due to diffraction, the beam spreads out This results in a situation in which the receiver aperture is only able to collect a fraction of the beam.
The remaining uncollected beam then results in beam divergence loss
: Diffraction limited beam divergence angle in radians
: Aperture diameter
In diffuse channels and FSO networks, is non-diffraction limited and determined by transmitter optics
: Radiation solid angle
Receiver effective antenna gain:
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Attenuation due to Beam Divergence
Transmitter effective antenna gain:
: Receiver effective aperture areas
Free-space path loss:
: Path length
For transmitted power , received power, , is (Friis transmission equation)
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Attenuation due to the Pointing Loss
When the received signal is not centered on the detector, a part of received signal may fall outside the detector area
Additional power penalty is usually incurred due to lack of perfect alignment of the transmitter and receiver
For short FSO links (
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