Published July 2010 | Version v1
Journal article

The correlated-k method and related methods for broadband radiation calculations

  • 1. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109 (United States)
  • 2. Harvard University, School of Engineering and Applied Sciences, Cambridge, MA 02138 (United States)

Description

The fundamentals of radiation calculations in planetary atmospheres have been known for a long time, but the practical problems of calculating radiation over a broad spectral range both efficiently and accurately remain an area of active research. The Goody et al. paper of 1989 established a milestone in that long effort. Goody et al. highlighted attempts to formulate the problem in terms of a few absorption coefficients that could represent typically tens of thousands of coefficients in a rigorous line-by-line calculation. Here we provide a brief background, point out that the correlated-k method is a special case of a broader spectral mapping concept, and mention some new ideas that have emerged recently.

Availability note (English)

Available from http://dx.doi.org/10.1016/j.jqsrt.2010.01.013

Additional details

Identifiers

DOI
10.1016/j.jqsrt.2010.01.013;
PII
S0022-4073(10)00024-5;

Publishing Information

Journal Title
Journal of Quantitative Spectroscopy and Radiative Transfer
Journal Volume
111
Journal Issue
11
Journal Page Range
p. 1672-1673
ISSN
0022-4073
CODEN
JQSRAE

INIS

Country of Publication
United Kingdom
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
44008311
Subject category
S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
Descriptors DEI
ABSORPTION; COMPUTERIZED SIMULATION; PLANETARY ATMOSPHERES
Descriptors DEC
ATMOSPHERES; SIMULATION; SORPTION

Optional Information

Copyright
Copyright (c) 2010 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.