Improved Determination of Ethane (C2H6) Abundance in Titan's Stratosphere

Author:

Livengood Timothy A.,Hewagama Tilak,Kostiuk Theodor,Fast Kelly E.,Goldstein Jeffrey J.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference19 articles.

1. Astrophysical Quantities;Allen,1976

2. Atakan, A. K, W. E. Blass, J. W. Brault, S. J. Daunt, G. W. Halsey, D. E. Jennings, D. C. Reuter, and, J. Susskind, 1983, The 12-Micron Band of Ethane: A Spectral Catalog from 765 cm−1 to 900 cm−1. NASA Technical Memorandum 85108, Goddard Space Flight Center, Greenbelt, Maryland.

3. The wavelength dependence of seeing;Boyd;J. Opt. Soc. Am.,1978

4. Nitrogen-broadened lines of ethane at 150 K;Chudamani;J. Quant. Spectrosc. Radiat. Transfer,1985

5. Titan's atmosphere from Voyager infrared observations. IV. Latitudinal variations of temperature and composition;Coustenis;Icarus,1995

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