ITU-R P 1817-1-2012 Propagation data required for the design of terrestrial free-space optical links《地面自由空间光链路设计的传播数据要求》.pdf

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1、 Recommendation ITU-R P.1817-1(02/2012)Propagation data required for the designof terrestrial free-space optical linksP SeriesRadiowave propagationii Rec. ITU-R P.1817-1 Foreword The role of the Radiocommunication Sector is to ensure the rational, equitable, efficient and economical use of the radio

2、-frequency spectrum by all radiocommunication services, including satellite services, and carry out studies without limit of frequency range on the basis of which Recommendations are adopted. The regulatory and policy functions of the Radiocommunication Sector are performed by World and Regional Rad

3、iocommunication Conferences and Radiocommunication Assemblies supported by Study Groups. Policy on Intellectual Property Right (IPR) ITU-R policy on IPR is described in the Common Patent Policy for ITU-T/ITU-R/ISO/IEC referenced in Annex 1 of Resolution ITU-R 1. Forms to be used for the submission o

4、f patent statements and licensing declarations by patent holders are available from http:/www.itu.int/ITU-R/go/patents/en where the Guidelines for Implementation of the Common Patent Policy for ITU-T/ITU-R/ISO/IEC and the ITU-R patent information database can also be found. Series of ITU-R Recommend

5、ations (Also available online at http:/www.itu.int/publ/R-REC/en) Series Title BO Satellite delivery BR Recording for production, archival and play-out; film for television BS Broadcasting service (sound) BT Broadcasting service (television) F Fixed service M Mobile, radiodetermination, amateur and

6、related satellite services P Radiowave propagation RA Radio astronomy RS Remote sensing systems S Fixed-satellite service SA Space applications and meteorology SF Frequency sharing and coordination between fixed-satellite and fixed service systems SM Spectrum management SNG Satellite news gathering

7、TF Time signals and frequency standards emissions V Vocabulary and related subjects Note: This ITU-R Recommendation was approved in English under the procedure detailed in Resolution ITU-R 1. Electronic Publication Geneva, 2012 ITU 2012 All rights reserved. No part of this publication may be reprodu

8、ced, by any means whatsoever, without written permission of ITU. Rec. ITU-R P.1817-1 1 RECOMMENDATION ITU-R P.1817-1*Propagation data required for the design of terrestrial free-space optical links (Question ITU-R 228/3) (2007-2012) Scope This Recommendation provides propagation data required for th

9、e design of free-space optical (FSO) links and planning of free-space optical systems, in the respective ranges of validity indicated in the Recommendation. The ITU Radiocommunication Assembly, considering a) that the visible optical and infrared spectrum is available for radiocommunications in the

10、Earths environments; b) that for the proper planning of free-space optic (FSO) radiocommunication systems operating in visible optical and infrared spectrum, it is necessary to have appropriate propagation data; c) that methods have been developed that allow the calculation of the most important pro

11、pagation parameters needed in planning free-space optical systems operating in visible optical and infrared spectrum; d) that, as far as possible, these methods have been tested against available data and have been shown to yield an accuracy that is both compatible with the natural variability of pr

12、opagation phenomena and adequate for most present applications in the planning of systems operating in the visible optical and infrared spectrum, recognizing a) that No. 78 of Article 12 of the ITU Constitution states that a function of the Radiocommunication Sector includes, “. carrying out studies

13、 without limit of frequency range and adopting recommendations .”, recommends 1 that the methods for predicting the propagation parameters given in Annex 1 should be adopted for planning free-space optical systems, in the respective ranges of validity indicated in the Annex. NOTE 1 Supplementary inf

14、ormation related to propagation prediction methods for frequencies in visible and infrared spectrum may be found in an ITU-R Recommendation on prediction methods required for the design of terrestrial free-space optical links. *This Recommendation should be brought to the attention of Radiocommunica

15、tion Study Groups 1 and 5. 2 Rec. ITU-R P.1817-1 Annex 1 1 Atmospheric considerations FSO links are impaired by absorption and scattering of light by the Earths atmosphere. The atmosphere interacts with light due to the composition of the atmosphere, which normally consists of a variety of different

16、 molecular species and small suspended particles called aerosols. This interaction produces a wide variety of phenomena: frequency selective absorption, scattering, and scintillation. Frequency selective absorption at specific optical wavelengths results from the interaction between the photons and

17、atoms or molecules that leads to the extinction of the incident photons, elevation of the temperature, and radiative emission. Atmospheric scattering results from the interaction between the photons and the atoms and molecules in the propagation medium. Scattering causes an angular redistribution of

18、 the radiation with or without modification of the wavelength. Scintillation results from thermal turbulence within the propagation medium that results in randomly distributed cells. These cells have variable sizes (10 cm-1 km), temperatures, and refractive indices causing scattering, multipath and

19、variation of the angles of arrival. As a result, the received signal amplitude fluctuates at frequencies ranging between 0.01 and 200 Hz. Scintillation also causes wave front distortion resulting in defocusing of the beam. In addition, sunlight can affect FSO performance when the sun is co-linear wi

20、th the direction of the free-space optical link. 2 Molecular absorption Molecular absorption results from an interaction between the optical radiation and the atoms and molecules of the medium (N2, O2, H2, H2O, CO2, O3, Ar, etc.). The absorption coefficient depends on the type and concentration of g

21、as molecules. The spectral variations of the absorption coefficient determine the absorption spectrum. The nature of this spectrum is due to the variations of possible energy levels of the gas generated essentially by the electronic transitions, vibrations of the atoms, and rotation of the molecules

22、. An increase in the pressure or temperature tends to widen the spectral absorption lines by excitation of higher energy levels and by the Doppler effect. Molecular absorption is a selective phenomenon that results in relatively transparent atmospheric transmission windows, and relatively opaque atm

23、ospheric absorption bands. The transmission windows in the optical range are: Visible and very-near IR: from 0.4 to 1.4 m Near IR or IR I: from 1.4 to 1.9 m and 1.9 to 2.7 m Mean IR or IR II: from 2.7 to 4.3 m and 4.5 to 5.2 m Far IR or IR III: from 8 to 14 m Extreme IR or IR IV: from 16 to 28 m. Th

24、e gaseous molecules have quantified energy levels proper to each species, and can absorb energy (or photons) under the influence of an incident electromagnetic radiation and transition from an initial energy level, ei, to a higher energy level, ef. The radiation energy is then attenuated by the loss

25、 of one or more photons. Rec. ITU-R P.1817-1 3 This process only occurs if the incident wave frequency corresponds exactly to one of the resonance frequencies of the considered molecule, given by: heeif=0(1) where: 0: incident wave frequency (Hz); h: Plancks constant, h = 6.6262 1034J-s. The fundame

26、ntal parameters that determine the absorption generated by molecular resonance are: the possible energy levels for each molecular species the probability of transition from an energy level eito an energy level ef, the intensity of resonance lines, and the natural profile of each line. Generally, the

27、 profile of each absorption line is modified by the Doppler effect when the molecules are moving relative to the incident wave, and by the collision effect due to the interaction of the molecules. These phenomena lead to a spectral widening of the natural line of each molecule. For certain molecules

28、, such as in carbon dioxide (CO2), water vapour (H2O), nitrogen (N2) and oxygen (O2), the absorption line profiles can extend sufficiently far from each central line. This property leads to an absorption continuum. Figure 1 shows the nominal measured atmosphere transmittance due to molecular absorpt

29、ion on a 1 820 m horizontal link at sea level. FIGURE 1 Transmittance of the atmosphere due to molecular absorption Wavelength (micrometers)023 8106040200Transmittance(%)8010014576 9 11 12 13 14 15Near infra red Mean infra red Far infra redO2H2OCO2CO2H2OH2OO2CO2O2H2OCO2CO23 Molecular scattering Mole

30、cular scattering results from the interaction of light with atmospheric particles whose sizes are smaller than the wavelength of the incident light. Scattering by atmospheric gas molecules (Rayleigh scattering) contributes to the total attenuation of the electromagnetic radiation. 4 Rec. ITU-R P.181

31、7-1 The extinction coefficient due to molecular scattering, m(), is: +=76362)(1)(1024)(22343nnm(2) where: m(): molecular scattering coefficient (km1); : wavelength (m); : molecular density (m3); : depolarization factor of the air ( 0.03); n(): refractive index of air. An approximate value of m() is:

32、 4)(= Am(3) where: TTPPA0031009.1= km1m4(4) and P: atmospheric pressure (mbar); P0: 1 013 mbar; T: atmospheric temperature (K); and T0: 273.15 K. Molecular scattering is negligible at infrared wavelengths, and Rayleigh scattering primarily affects ultraviolet wavelengths up to visible wavelengths. T

33、he blue colour of the clear-sky background is due to this type of scattering. 4 Aerosol absorption Aerosols are extremely fine solids or liquids particles suspended in the atmosphere with very low fall speed (ice, dust, smoke, etc). Their size generally lies between 102and 100 m. Fog, dust and marit

34、ime spindrift particles are examples of aerosols. Aerosols influence the conditions of atmospheric attenuation due to their chemical nature, their size and their concentration. In maritime environments, the aerosols are primarily made up of droplets of water (foam, fog, drizzle, rain), salt crystals

35、, and various particles of continental origin. The type and density of continental particles depend on the distance from, and characteristics of, the neighbouring coasts. The extinction coefficient due to aerosol absorption, n(), is: drdrrdNrnrQan)(“,210)(205=km1(5) Rec. ITU-R P.1817-1 5 where: : wa

36、velength (m); dN(r)/dr: particle size distribution per unit of volume (cm4); n: imaginary part of the refractive index, n, of the considered aerosol; r: radius of the particles (cm); Qa(2r/, n): absorption cross-section for a given type of aerosol. Mie theory predicts the electromagnetic field diffr

37、acted by homogeneous spherical particles. The absorption (Qa)and scattering (Qd) cross-sections depend on the particle size, refractive index and incident wavelength. They represent the portion of an incident wave where the absorbed (scattered) power is equal to the incident power. The refractive in

38、dex of aerosols depends on their chemical composition and the wavelength. It is denoted as n = n + n where is n is a function of the scattering capacity of the particle, and n is a function of the absorption of the particle. In the visible and near infrared spectral regions, the imaginary part of th

39、e refractive index is extremely low and can be neglected in the calculation of global attenuation (extinction). In the far infrared case, the imaginary part of the refractive index must be taken into account. 5 Aerosol scattering Aerosol scattering (Mie scattering) occurs when the particle size is t

40、he same order of magnitude as the wavelength of the incident light. Attenuation is a function of frequency and visibility, and visibility is related to the particle size distribution. This phenomenon constitutes the most restrictive factor to the deployment of free-space optical systems at long dist

41、ances. In the optical region, it is mainly caused by mist and fog. The attenuation in the optical regime can reach 300 dB/km, in contrast to the millimetre wave region, where rain attenuation is typically a few dB/km. The extinction coefficient due to aerosol scattering, n, is given by the following

42、 relation: drdrrdNrnrQdn=025)(,210)( km1(6) where: : wavelength (m); dN(r)/dr: particle size distribution per unit of volume (cm4); n: real part of the refractive index n of the aerosol; r: radius of the particles (cm); Qd(2r/, n): scattering cross-section for a given type of aerosol. Mie theory pre

43、dicts the scattering coefficient Qddue to the aerosols, assuming the particles are spherical and sufficiently separated so that the scattered field can be calculated assuming far field (single) scattering. The scattering cross-section Qdstrongly depends on the size of the aerosol compared to the wav

44、elength, and is a very frequency-selective function for particles whose radius is less than or equal to the wavelength. It reaches its maximum value (3.8) for a particle radius equal to the wavelength, in which case the scattering is maximal. As the size of the particle increases, the scattering cro

45、ss-section asymptotes to a value approximately equal to 2. 6 Rec. ITU-R P.1817-1 Since the aerosol concentration, composition and size distribution vary temporally and spatially, it is difficult to predict attenuation by these aerosols. Although the concentration is closely related to the optical vi

46、sibility, there is not a unique particle size distribution for a given visibility. Visibility characterizes the transparency of the atmosphere as estimated by a human observer. It is measured by the runway visual range (RVR), and is the distance that a luminous beam must travel through the atmospher

47、e for its intensity (or luminous flux) to drop to 0.05 times its original value. It may be measured using a transmissometer or a diffusiometer. Figure 2 gives an example of the variations of the runway visual range observed at La Turbie, France, during a day with high visibility. FIGURE 2 Variations

48、 of the runway visual range observed at La Turbie (France) during a day with high visibility Hour00:00 05:59 17:591.51.00.50.0Runwayvisualrange(m)2.02.511:59 23:593.03.54.04.55.05.5 10424/03/02Alternatively, visibility along the transmission path can be measured using a CCD camera and a black and wh

49、ite reference target. For this method, the visual range, Vr, is given by: dCCVr)/(In)02.0(In0= (7) Rec. ITU-R P.1817-1 7 C is the measured contrast between the black and white regions of the target, C0is the intrinsic contrast ratio of the target (measured close to it), and d is the distance to the target. The value of C is given by the relation: rEXVbbwbweLLLLC=+= 02.0 (8) where Lwand Lbare the luminance of the white and black parts of the target, bEX