Titan's stratospheric zonal wind, temperature, and ethane abundance a year prior to Huygens insertion-Reference-Cited by-同舟云学术

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Titan's stratospheric zonal wind, temperature, and ethane abundance a year prior to Huygens insertion

Published:2005-11 Issue:22 Volume:32 Page:n/a-n/a
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophys. Res. Lett.

Author:

Kostiuk T.¹,Livengood T. A.¹,Hewagama T.¹,Sonnabend G.²,Fast K. E.¹,Murakawa K.³,Tokunaga A. T.⁴,Annen J.¹,Buhl D.¹,Schmülling F.⁵

Affiliation:

1. NASA Goddard Space Flight Center; Greenbelt Maryland USA

2. National Research Council; NASA Goddard Space Flight Center; Greenbelt Maryland USA

3. Subaru Telescope; National Astronomical Observatory of Japan; Hilo Hawaii USA

4. Institute for Astronomy; University of Hawaii; Honolulu Hawaii USA

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

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Reference28 articles.

1. The Huygens Doppler wind experiment-Titan winds derived from probe radio frequency measurements;Bird;Space Sci. Rev.,2002

2. Bouchez , A. H. 2004 Seasonal trends in Titan's atmosphere: Haze, wind, and clouds 52 91 Calif. Inst. of Technol. Pasadena

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

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

5. Titan's atmosphere from ISO mid-infrared spectroscopy;Coustenis;Icarus,2003

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