A non-local thermodynamic equilibrium radiative transfer model for infrared emissions in the atmosphere of Mars: 2. Daytime populations of vibrational levels-Reference-Cited by-同舟云学术

A non-local thermodynamic equilibrium radiative transfer model for infrared emissions in the atmosphere of Mars: 2. Daytime populations of vibrational levels

Published:1994 Issue:E6 Volume:99 Page:13117
ISSN:0148-0227
Container-title:Journal of Geophysical Research
language:en
Short-container-title:J. Geophys. Res.

Author:

Lopèz-Valverde M. A.,Lopèz-Puertas M.

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Link

http://www.agu.org/journals/je/v099/iE06/94JE01091/94JE01091.pdf

Reference14 articles.

1. Dayside temperatures of the Martian upper atmosphere;Bittner;J. Geophys. Res.,1987

2. Mars mesosphere and thermosphere, 1, Global mean heat budget and thermal structure;Bougher;J. Geophys. Res.,1988

3. Modeling of the 10 μm natural laser emission from the mesospheres of Mars and Venus;Deming;Icarus,1983

4. Observations of the 10 μm natural laser emission from the mesospheres of Mars and Venus;Deming;Icarus,1983

5. A high-resolution atlas of the infrared spectrum of the Sun and the Earth's atmosphere from space;Farmer,1989

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