Paper
31 October 1996 Reviewing atmospheric radiative transfer modeling: new developments in high- and moderate-resolution FASCODE/FASE and MODTRAN
Gail P. Anderson, F. X. Kneizys, James H. Chetwynd Jr., Laurence S. Rothman, Michael L. Hoke, Alexander Berk, Lawrence S. Bernstein, Prabhat K. Acharya, Hilary E. Snell, Eli Mlawer, Shepard A. Clough, Jinxue Wang, Szu-Chia Lee, Henry E. Revercomb, Tatsuya Yokota, L. M. Kimball, Eric P. Shettle, Leonard W. Abreu, John E. A. Selby
Author Affiliations +
Abstract
Spectrally uniform treatment of the atmospheric radiative transfer (RI) problem has been approached through two different techniques - very high resolution line-by-line (LBL) algorithms and lower resolution band models (BM). Each has its advantages and specific applications. However, if commonality and validation of a specific pair of RI approaches is to be mutually maintained, then these codes must be continually reevaluated against both measurements and other models.
© (1996) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Gail P. Anderson, F. X. Kneizys, James H. Chetwynd Jr., Laurence S. Rothman, Michael L. Hoke, Alexander Berk, Lawrence S. Bernstein, Prabhat K. Acharya, Hilary E. Snell, Eli Mlawer, Shepard A. Clough, Jinxue Wang, Szu-Chia Lee, Henry E. Revercomb, Tatsuya Yokota, L. M. Kimball, Eric P. Shettle, Leonard W. Abreu, and John E. A. Selby "Reviewing atmospheric radiative transfer modeling: new developments in high- and moderate-resolution FASCODE/FASE and MODTRAN", Proc. SPIE 2830, Optical Spectroscopic Techniques and Instrumentation for Atmospheric and Space Research II, (31 October 1996); https://doi.org/10.1117/12.256105
Lens.org Logo
CITATIONS
Cited by 21 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Atmospheric modeling

Transmittance

Absorption

Radiative transfer

Spectroscopy

Multiple scattering

Solar radiation models

Back to Top