High spatial resolution mapping of Mars mesospheric zonal winds by infrared heterodyne spectroscopy of CO2

Author:

Sonnabend G.12,Sornig M.12,Krötz P. J.12,Schieder R. T.12,Fast K. E.23

Affiliation:

1. I. Physikalisches Institut; Universität zu Köln; Cologne Germany

2. Visiting Astronomer; National Solar Observatory; Tucson Arizona USA

3. NASA Goddard Space Flight Center; Greenbelt Maryland USA

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Reference23 articles.

1. The first Mars thermospheric general circulation model: The Martian atmosphere from the ground to 240 km;Angelats i Coll;Geophys. Res. Lett.,2005

2. Clancy , R. T. B. J. Sandor G. H. Moriarty-Schieven M. D. Smith 2006 Mesospheric winds and temperatures from JCMT sub-millimeter CO line observations during the 2003 and 2005 Mars oppositions 2nd Workshop on Mars Atmosphere Modelling and Observations Granada, Spain

3. Observations of the 10-micron natural laser emission from the mesospheres of Mars and Venus;Deming;Icarus,1983

4. Edwards , D. P. 1992 GENLN2: A general line-by-line atmospheric transmittance and radiance model Rep. NCAR/TN-367+STR Natl. Cent. for Atmos. Res. Boulder, Colo.

5. Ozone abundance on Mars from infrared heterodyne spectra Acquisition, I., retrieval, and anticorrelation with water vapor;Fast;Icarus,2006

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