Abstract
The Martian temperature fields simulated with general circulation models are used to calculate the CO spectra in the submillimeter wavelength (691GHz). In the spectra within the offset frequency of ±500MHz, we can see the information of temperature from the planetary surface to ~80km height atmosphere. The difference of the spectra obtained from the temperature fields in different seasons and models are discussed, for the upcoming submillimeter observations of the Martian atmosphere.
Original language | English |
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Title of host publication | Advances in Geosciences |
Subtitle of host publication | Volume 15: Planetary Science (PS) |
Publisher | World Scientific Publishing Co. |
Pages | 17-24 |
Number of pages | 8 |
ISBN (Electronic) | 9789812836229 |
ISBN (Print) | 9812836101, 9789812836212 |
DOIs | |
Publication status | Published - 2009 Jan 1 |
Externally published | Yes |
ASJC Scopus subject areas
- Earth and Planetary Sciences(all)
- Physics and Astronomy(all)