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C path: /stormrc1/aer_lblrtm/src/SCCS/s.lblrtm_instructions C revision: 5.8 C created: 11/10/99 14:22:09 C presently: 11/10/99 14:23:17 PRELIMINARY USER INSTRUCTIONS FOR LBLRTM 01 November 1999 RECORD 1.1 CXID: 80 characters of user identification (80A1) CXID(1) is the flag which determines program
19 Oct 2017 (M. J. Alvarado); Updated lblrtm instructions. C path: /stormrc1/aer_lblrtm/src/SCCS/s.lblrtm_instructions C revision: 5.8 C created: 11/10/99 14:22:09 C presently: 11/10/99 14:23:17 PRELIMINARY USER 11 Sep 2009 This is a lot easier than figuring out what's written in the manual lblrtm_instructions.
11 Sep 2009 These wrapper functions will process standard user inputs and create TAPE5 files and run LBLRTM. This is a lot easier than figuring out what's written in the manual lblrtm_instructions. LBLRTM stands for Line-by-Line Radiative Transfer model. It is an advanced and highly-configurable radiative transfer
PyLBLRTM - Helper functions in reading/writing LBLRTM input/output files. PyLBLRTM is a collection of Python scripts to ease the use of the line-by-line radiative transfer model (LBLRTM) managed by AER. These scripts allow for the following: 1.) Creation of the input ###Installation Instructions. Type: python setup.py
9 Jul 2007 the MPTS/NPTS options of TAPE5 record 1.2. 4 Instructions and Tips for Running LNFL. LNFL is used to generate a unformatted file (TAPE3) of all the line parameters required by. LBLRTM. 4.1 Input files for LNFL. TAPE1: The line parameter database in ASCII format (also available on wwwrtweb.aer.com).
Author : $Author: jdelamer $ Revision : $Revision: 1.5 $ Created : $Date: 2011/03/02 18:33:23 $ INSTRUCTIONS FOR LINE FILE CREATION FOR LBLRTM LNFL LNFL now accommodates the 160 character format adopted for HITRAN_2004. However, the default format for LNFL will remain the 100 character format.
LBLRTM - The Line-By-Line Radiative Transfer Model is an accurate, efficient and highly flexible model for calculating spectral transmittance and radiance. See also[edit]. List of atmospheric radiative transfer codes · Atmospheric radiative transfer codes · Absorption spectrum · HITRAN. References[edit]. Clough, S. A., M. W.
(S.A. Clough and Paolo Antonelli); Fixed a documentation error in the LBLRTM instructions. (K.E. Cady-Pereira). Fixed a coding error is the solar source function. (K.E. Cady-Pereria and S. Ferron). Modified LBLRTM to handle underflow problem in convolution routine. (M.W. Shephard, S.A. Clough, G. Uymin). Modified the
In short, however, all of the instructions are passed into the LBLRTM via an input file that we will affectionately call the TAPE5. This is historical, back when the original LOWTRAN model was designed to take input from punch cards. The TAPE5 is an ascii file, but it is very format specific: being off even one space can cause
31 Oct 2011 3 Instructions and Tips for Running LNFL. LNFL is used to generate a unformatted file (TAPE3) of all the line parameters required by LBLRTM. 3.1 Input files for LNFL. TAPE1: The line parameter database in ASCII format (also available on wwwrtweb.aer.com). TAPE5: LNFL input file. 3.2 Output files for
     

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