6SV

 

adapted from Vermote et al., (1997) and 6SV site.

6SV

Conceptual representation of 6SV radiative transfer.

 

The 6S (Second Simulation of the Satellite Signal in the Solar Spectrum) (Vermote et al., 1997) is a computer code that can accurately simulate the radiative transfer of an optical electromagnetic signal through the atmosphere. The 6S code is an improved version of 5S, developed by the Laboratoire d’Optique Atmospherique, that permits calculations of near-nadir (down-looking) aircraft and satellite observations, accounting for target elevation, non lambertian surface conditions, and absorbing species (O2, O3, H2O, CH4, N2O, CO). The computational accuracy for Rayleigh and aerosol scattering effects is based on the use of state-of-the-art approximations and implementation of the successive order of scattering (SOS) algorithm. 6S simulates the atmospheric radiative transfer in the 400-2500 nm spectral range at a spectral resolution of 2.5 nm.

Nevertheless, the 6S code has still limitations. It cannot handle spherical atmosphere and as a result, it cannot be used for limb observations. In addition, the decoupling we are using for absorption and scattering effects does not allow to use the code in presence of strong absorption bands.

Our Atmospheric LUT Generator (ALG) toolbox v. 1,2 supports usage of the latest vector version of the 6S code (6SV2.1) (Kotchenova et al., 2006, Kotchenova et al., 2007, Kotchenova et al., 2008). 6SV2.1 was released in June 2015, and is available to download here.

 

Contact:

  • Eric V. VERMOTE, Terrestrial Information Systems Laboratory NASA GSFC, Code 619, Greenbelt, MD, USA
  • S.Y. KOTCHENOVA, Department of Earth and Environment Boston University, Boston, USA
  • D. TANRÉ, J.L. DEUZÉ and M. HERMAN, Laboratoire d' Optique Atmosphérique Université des Sciences et Techniques de Lille U.E.R. de Physique Fondamentale 59655 Villeneuve d' Ascq Cedex, France
  • J-C. ROGER, Department of Geographical Sciences University of Maryland, College Park, MD, USA and Terrestrial Information Systems Laboratory NASA GSFC, Code 619, Greenbelt, MD, USA
  • J.J. MORCRETTE, European Center for Medium - Range Weather Forecasting Shinfiels Park, Reading Bershire RG2 9AX, United Kingdom
  • R. MATARRESE, 6S Interface Credit Department of Physics University of Bari, Bari, Italy

References: