An improved model of radiative transfer for the NLTE problem in the NIR bands of CO2 and CO molecules in the daytime atmosphere of Mars. 1. Input data and calculation method
Author:
Publisher
Pleiades Publishing Ltd
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/content/pdf/10.1134/S003809461605004X.pdf
Reference68 articles.
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3. Billebaud, F., Crovisier, J., Lellouch, E., Encrenaz, T., and Maillard, J.P., High-resolution infrared spectrum of CO on Mars: evidence for emission lines, Planet. Space Sci., 1991, vol. 39, pp. 213–218.
4. Bougher, S.W., Pawlowski, D., Bell, J.M., Nelli, S., McDunn, T., Murphy, J.R., Chizek, M., and Ridley, A., Mars Global Ionosphere-Thermosphere Model: solar cycle, seasonal, and diurnal variations of the Mars upper atmosphere, J. Geophys. Res. E, 2015, vol. 120, pp. 311–342. doi 10.1029/2014JE004715
5. Brechignac, Ph., Near-resonant V-V transfer rates for highlying vibrational states of CO, Chem. Phys., 1978, vol. 34, pp. 119–134.
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