Comparison of line-by-line and band-model calculations of methane absorption in outer planet atmospheres.

Details Comparison of line-by-line and band-model calculations of methane absorption in outer planet atmospheres. Comparison of line-by-line and band-model calculations of methane absorption in outer planet atmospheres.

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1384s&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1384

Computer Science

Scientific paper

Recent improvements in the measurement of methane absorption lines at wavenumbers in the region between 4800 cm-1 and 7700 cm-1 have greatly increased the number of lines with known ground-state energies, the number of weak lines, and the number of lines observed at low temperatures. This has made it possible to create a low-temperature line list that allows modeling near IR spectra of Titan using line-by-line calculations instead of band models [1]. Here, we compare current band models with line-by-line calculations, both to assess the behavior of band models, and to identify remaining issues with line-by-line calculations when applied to outer planet atmospheres.

Affiliated with

Also associated with

No associations

Rating

Comparison of line-by-line and band-model calculations of methane absorption in outer planet atmospheres. does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Comparison of line-by-line and band-model calculations of methane absorption in outer planet atmospheres., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Comparison of line-by-line and band-model calculations of methane absorption in outer planet atmospheres. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1484540