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6S用户手册
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6S模型用户手册,适合新手学习了解6S的原理和使用,内部包含代码示例
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Second Simulation of a Satellite Signal
in the Solar Spectrum - Vector (6SV)
Vermote E.
(1,*)
, D. Tanré
(2)
, J. L. Deuzé
(2)
, M. Herman
(2)
,
J. J. Morcrette
(3)
, and S. Y. Kotchenova
(1)
(1) Department of Geography, University of Maryland
address for correspondence:
4321 Hartwick Road, Suite 209
College Park, MD 20740
(2) Laboratoire d'Optique Atmosphérique, URA CNRS 713
Université des Sciences et Technologies de Lille
59655 Villeneuve d'Ascq Cédex, France
(3) European Centre for Medium Range Weather Forecast
Shinfield Park, Reading
Berkshire RG2 9AX, United Kingdom
* Formerly affiliated with the Laboratoire d'Optique Atmosphérique
![](https://csdnimg.cn/release/download_crawler_static/10403375/bg2.jpg)
6S User Guide Version 3, November 2006
2
CONTENTS
ABSTRACT 3
UPDATES 4
HISTORY 5
PHYSICAL BACKGROUND 6
DESCRIPTION OF ATMOSPHERIC EFFECTS IN SATELLITE OBSERVATIONS 10
1. Absorbing effects 10
2. Scattering effects 11
2.1. Case of a Lambertian uniform target 11
2.2. Environmental function 14
2.3. Intrinsic atmospheric reflectance 16
2.4. Airplane and elevated target simulations 18
2.5. Directional effect of the target 20
2.6. Atmospheric correction scheme 22
3. Interaction between absorption and scattering effects 23
CONCLUSION 26
FIGURES 27
ACKNOWLEDGMENTS 31
APPENDIX
I. Description of the computer code 32
II. Examples of inputs and outputs 52
III. Description of the subroutines 56
![](https://csdnimg.cn/release/download_crawler_static/10403375/bg3.jpg)
6S User Guide Version 3, November 2006
3
ABSTRACT
This is the manual for a vector version of the 6S radiative transfer (RT) code (hereafter also
referred to as 6SV), capable of accounting for radiation polarization. The manual presents a
modified version of the previous scalar 6S manual. For the user’s convenience, the format and
style of this new manual have been kept as close as possible to those of the previous version.
6S - Second Simulation of a Satellite Signal in the Solar Spectrum - is a basic RT code used
for the calculation of look-up tables in the MODIS (MODerate resolution Imaging Spectro-
radiometer) atmospheric correction algorithm. It enables accurate simulations of satellite and
plane observations, accounting for elevated targets, modeling of a realistic molecular/aerosol/
mixed atmosphere, use of Lambertian/anisotropic ground surfaces, and calculation of gaseous
absorption. It is one of the most widely used, rigorously validated, and heavily documented RT
codes known in the scientific remote-sensing community.
The latest updates on the code status (dated May 2005) include a public release of its vector
version, 6SV1.0B. As its scalar predecessors, the vector version is based on the method of
successive orders of scattering (SOS) approximations. The effects of polarization are included
through the calculation of four components of the Stokes vector, characterizing the intensity of
radiation, and perpendicular, parallel, and elliptical polarization. The accuracy of RT calculations
can be varied by changing the number of calculation angles and layers. By default, 6SV1.0B uses
the “standard accuracy” conditions which provide the user with a relative average accuracy of
approximately 0.4-0.6%, compared to standard benchmarks and other RT codes.
![](https://csdnimg.cn/release/download_crawler_static/10403375/bg4.jpg)
6S User Guide Version 3, November 2006
4
UPDATES
The information on news and updates is posted on the 6S Web site at http://6s.ltdri.org. This
site also contains pdf-files of relevant publications.
I. News
1) A special Web interface which can help an inexperienced user learn how to use the code and
build necessary input files is available at the 6S Web site.
2) The paper “Validation of a vector version of the 6S radiative transfer code for atmospheric
correction of satellite data. Part II: Homogeneous Lambertian and anisotropic surfaces”, by S.Y.
Kotchenova, E.F. Vermote and P.A. Farris is submitted to Applied Optics in December, 2006.
3) 6SV is participating in the joint RT scalar/vector code comparison project, which the MODIS
atmospheric correction group performs together with the NASA Goddard Space Flight Center,
http://rtcodes.ltdri.org.
II. Changes
Scalar version of 6S Vector version of 6S
1. Scalar (ignoring the effects of polarization) 1. Vector (accounting for polarization)
2. Fixed number of scattering angles (83), used
for the specification of an aerosol phase
function
2. Ability to vary the number of scattering
angles (up to 1000)
3. 10 node wavelengths 3. 20 node wavelengths
4. Fixed number of calculation layers (26) and
angles (48)
4. Ability to change the number of calculation
layers and angles
5. Default exponential vertical aerosol profile 5. Default exponential + user-defined (up to 50
layers in the height range 0-100 km) vertical
aerosol profiles
6. Several new subroutines, simulating measurements of the ALI, ASTER, ETM, HYPBLUE,
VGT, and VIIRS instruments, have been integrated into the vector 6S. These subroutines were
developed by Dr. T. Miura, University of Hawaii at Manoa, Honolulu, USA.
![](https://csdnimg.cn/release/download_crawler_static/10403375/bg5.jpg)
6S User Guide Version 3, November 2006
5
HISTORY
July 1992 Development of the scalar 5S (Simulation of a Satellite Signal in the Solar
Spectrum) RT code by le Laboratoire d’Optique Atmosphérique.
July 1997 Release of a new improved version of the 5S code, called 6S (Second
Simulation of a Satellite Signal in the Solar Spectrum). 6S becomes a basic RT
code used for the calculation of look-up tables in the MODIS atmospheric
correction algorithm.
May 2005 Release of a vector version of 6S, capable of accounting for radiation
polarization.
October 2005 Organization of a joint scalar/vector RT code comparison project together with
the NASA Goddard Space Flight Center.
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