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Solar radiation extinction in the atmosphere

Содержание

Incoming SRWhen passing through the atmosphere SR undergoes significant changes Incoming SRDiffused part of SRAbsorbed part of SR

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Слайд 1Solar radiation extinction in the atmosphere
Lecture 3

Solar radiation extinction in the atmosphereLecture 3

Слайд 2Incoming SR
When passing through the atmosphere SR undergoes significant changes







Incoming SR
Diffused part of SR
Absorbed part of SR

Incoming SRWhen passing through the atmosphere SR undergoes significant changes Incoming SRDiffused part of SRAbsorbed part of

Слайд 3Lecture 3
SR absorption
The main gases absorbing S radiation are Ozone

(O3), Oxygen (O2), Water vapor (H2O), and Carbon dioxide (CO2).
Ozone




Lecture 3SR absorptionThe main gases absorbing S radiation are Ozone (O3), Oxygen (O2), Water vapor (H2O), and

Слайд 4Lecture 3






Ozone (O3) absorbtion

Lecture 3Ozone (O3) absorbtion

Слайд 5Lecture 3
Oxygen
Water vapor

Carbon dioxide
0,13 – 0,24
0,72; 0,84; 0,94; 1,14; 1,38;

1,87; 2,7; 3,2

1,44; 1,6; 2,02; 2,7; 4,31;


Lecture 3OxygenWater vaporCarbon dioxide0,13 – 0,240,72; 0,84; 0,94; 1,14; 1,38; 1,87; 2,7; 3,21,44; 1,6; 2,02; 2,7; 4,31;

Слайд 6Lecture 3
http://en.wikipedia.org/wiki/File:Atmospheric_Transmission.png
http://en.wikipedia.org/wiki/File:Atmospheric_Transmission.png

Lecture 3http://en.wikipedia.org/wiki/File:Atmospheric_Transmission.pnghttp://en.wikipedia.org/wiki/File:Atmospheric_Transmission.png

Слайд 7Lecture 3
Water vapor transmission function

Qv is the mass of water

vapor in a column of air with the base 1

bi and βi are quantities empirically obtained.

Mass of the water vapor in the atmosphere is larger than that of ozone and carbon dioxide. Hence, it absorbs the larger part of the total absorbed radiation.

Nitrogen does not absorb radiation. Solid aerosols also absorb SR. In the layer 0,3 – 8,4 km O2 and CO2 absorb 3,8% and solid aerosols absorb 4,8% of SR.


Lecture 3Water vapor transmission functionQv is the mass of water vapor in a column of air with

Слайд 8Lecture 3
SR diffusion in the atmosphere
Terminology
Diffusion (произвольное рассеяние)
Scattering (Разбрасывание в

разных направлениях любых веществ, предметов и даже людей)
Dispersion (синоним Scattering,

в науке применяется к свету)
Turbidity (мутность).
The atmosphere is turbid medium due to many admixtures (aerosols) suspended in the air.
Aerosols scatter and absorb solar and terrestrial radiation.
Lecture 3SR diffusion in the atmosphereTerminologyDiffusion (произвольное рассеяние)Scattering (Разбрасывание в разных направлениях любых веществ, предметов и даже

Слайд 9Lecture 3
Molecular scattering or Rayleigh scattering
The atmosphere is turbid medium diffusing

SR even in the absence of aerosols. In this case

turbidity is molecular complexes.







The essence of the scattering is a particular form of interaction between variable field of coming electromagnetic waves and particles in the medium. Due to this kind of interaction the particles become sources of new electromagnetic waves.
































Lecture 3Molecular scattering or Rayleigh scatteringThe atmosphere is turbid medium diffusing SR even in the absence of

Слайд 10Lecture 3
John William Strutt, third Baron Rayleigh

"Lord Rayleigh - Biography".

Nobelprize.org. 22 Sep 2010 http://nobelprize.org/nobel_prizes/physics/laureates/1904/strutt-bio.html
1842 - 1919

Lecture 3John William Strutt, third Baron Rayleigh

Слайд 11Lecture 3
Rayleigh scattering

http://hyperphysics.phy-astr.gsu.edu/hbase/atmos/blusky.html#c4

Lecture 3Rayleigh scatteringhttp://hyperphysics.phy-astr.gsu.edu/hbase/atmos/blusky.html#c4

Слайд 12Lecture 3

Lecture 3

Слайд 13Lecture 3
Raman scattering
Rayleigh scattering can be considered to be elastic

scattering ( the photon energies of the scattered photons is

not changed)
Scattering in which the scattered photons have either a higher or lower photon energy is called Raman scattering.
Usually this kind of scattering involves exciting some vibrational mode of the molecules, giving a lower scattered photon energy, or scattering off an excited vibrational state of a molecule which adds its vibrational energy to the incident photon.
Lecture 3Raman scatteringRayleigh scattering can be considered to be elastic scattering ( the photon energies of the

Слайд 14Lecture 3
Raman scattering
C. V. Raman discovered the inelastic scattering phenomenon

which bears his name in 1928 and for it he

was awarded the Nobel Prize for Physics in 1930.
Lecture 3Raman scatteringC. V. Raman discovered the inelastic scattering phenomenon which bears his name in 1928 and

Слайд 15Lecture 3
Molecular scattering (Continuation)
The incident radiation flux of a definite wavelength

makes fluxes of the radiation of the same wavelength.
This process

is greatly influenced by the geometrical structure and properties of the turbid medium. The geometrical structure is determined by dimensionless parameters and The laws of scattering are quite different for the

cases and .

If , the particles can be regarded as independent emittants.
The phenomenon of interference will not be observed.
No additional fields of radiation will appear.
Instead, the intensities of the radiation will be summed up. This simplifies solution of the problem of, so called, multiple scattering.
















Lecture 3Molecular scattering (Continuation)The incident radiation flux of a definite wavelength makes fluxes of the radiation of

Слайд 16Lecture 3
Multiple scattering
Multiple scattering is the result of diffusion of

the previously scattered radiation.
Multiple scattering can be neglected if the

medium turbidity is not very high, i. e. the scattering particles are very distant from each other
Lecture 3Multiple scatteringMultiple scattering is the result of diffusion of the previously scattered radiation.Multiple scattering can be

Слайд 17Lecture 3
Physical properties of the scattering fields
The main characteristics of

the properties is complex index of refraction.

is absolute index of

refraction
is characteristics of absorption
The theory of the molecular scattering had been developed by English scientist Rayleigh, who put in the base of the theory the following assumptions:
All particles have form of a ball. They are dielectrically homogeneous and r<<λ.
Particle index of refraction does not markedly differ from that of the medium: nμ<1 and μ=2πr/λ.
The particles diffuse the light independently, I. e. L>>λ
The diffused light is observed at the distance R>>r






Lecture 3Physical properties of the scattering fieldsThe main characteristics of the properties is complex index of refraction.		is

Слайд 18Lecture 3
Aerosol scattering Mie theory (also called Lorenz–Mie theory or Lorenz–Mie–Debye

theory)
Aerosol particles are much larger than molecule complexes
There are

two types of the larger particles in the atmosphere: non-transparent ones (dust, ), and transparent ones (water droplets).

Water droplets absorb radiation of ultraviolet and visible parts of the spectrum just slightly. Absolute index of refraction for water droplets varies not significantly. It average value n=1,33.
n is absolute index of refraction

Lecture 3Aerosol scattering Mie theory (also called Lorenz–Mie theory or Lorenz–Mie–Debye theory)Aerosol particles are much larger than

Слайд 19Lecture 3
Gustav Mie, German physicist

1869 –1957

Lecture 3Gustav Mie,  German physicist1869 –1957

Слайд 20Lecture 3
The volume coefficient of extinction for larger particles

is a

function of quantity
m - complex index of refraction,
N

is the number of particles in a unit of volume.
For very large particles (10In case r>40 μ, the scattering does not depend on wavelength.


Lecture 3The volume coefficient of extinction for larger particles				is a function of quantity		 m - complex index

Слайд 21Lecture 3
If many particle of this size are present in

the atmosphere the sky becomes of whitish color (instead of

light blue) due to the fact that the light dispersed in the same way regardless which wavelength is dispersed.
Due to the same reason, clouds and fogs have white (whitish) or gre`y color.
Scatter indicatrix for several values of parameter μ.










4


30


8

The larger particles mainly scatter in the direction of incident beam

Lecture 3If many particle of this size are present in the atmosphere the sky becomes of whitish

Слайд 22Lecture 3
http://hyperphysics.phy-astr.gsu.edu/hbase/atmos/blusky.html#c4
Scatter indicatrix is a vectoral diagram depicting dependence of

scattered radiation on direction.
http://hyperphysics.phy-astr.gsu.edu/hbase/atmos/blusky.html#c4

Lecture 3http://hyperphysics.phy-astr.gsu.edu/hbase/atmos/blusky.html#c4Scatter indicatrix is a vectoral diagram depicting dependence of scattered radiation on direction. http://hyperphysics.phy-astr.gsu.edu/hbase/atmos/blusky.html#c4

Слайд 23Lecture 3
Simultaneous molecular and aerosol scattering
Since in the atmosphere

some kind of aerosols always exists, both molecular and aerosol

scattering goes on simultaneously.
It makes difficult to estimate real scattering quantitatively from the theoretically obtained equations. Instead some empirical or semi-empirical relations are used for the purpose. It was learnt that regularities of the scattering strongly depends upon the sizes of the particles, and, first of all, on the water droplet sizes.
Very important characteristics is so called scattering index Kλ.

Molecular scattering index

Aerosol scattering index

Prevails up to 3 – 4 km


Prevails above 3 – 4 km

depends on turbidity

depend on turbidity too

Lecture 3Simultaneous molecular and aerosol scattering Since in the atmosphere some kind of aerosols always exists, both

Слайд 24Lecture 3
Optical depth of the atmosphere
The volume extinction index summed

up through the whole atmosphere is termed optical depth of

the atmosphere.



is the optical depth caused by molecular scattering, and is that caused by the total scattering.
In the ultraviolet area (λ<40μ) the molecular scattering makes the larger contribution in the total scattering, at λ=0,45 both contribution are almost equal, at λ>0,45 aerosol scattering contribution prevails.

Lecture 3Optical depth of the atmosphereThe volume extinction index summed up through the whole atmosphere is termed

Слайд 25Lecture 3
What is the type of scattering below?
http://en.wikipedia.org/wiki/Rayleigh_scattering

The beam

of a 5 mW green laser pointer is visible at

night due to Rayleigh scattering and airborne dust.
Lecture 3What is the type of scattering below?http://en.wikipedia.org/wiki/Rayleigh_scattering The beam of a 5 mW green laser pointer

Слайд 26Lecture 3
Which type of scattering is presented? Рерих Н.К. “Величайшая и

Святейшая Тангла “

Lecture 3Which type of scattering is presented?  Рерих Н.К. “Величайшая и Святейшая Тангла “

Слайд 27Lecture 3
Beijing’s sky

Lecture 3Beijing’s sky

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