The implications of the H2variability in Titan's exosphere-Reference-Cited by-同舟云学术

The implications of the H2variability in Titan's exosphere

Published:2011-11 Issue:A11 Volume:116 Page:n/a-n/a
ISSN:0148-0227
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res.

Author:

Cui J.¹²,Yelle R. V.³,Müller-Wodarg I. C. F.⁴,Lavvas P. P.³,Galand M.⁴

Affiliation:

1. Department of Astronomy and Key Laboratory of Modern Astronomy and Astrophysics, Ministry of Education; Nanjing University; Nanjing China

2. National Astronomical Observatories; Chinese Academy of Sciences; Beijing China

3. Lunar and Planetary Laboratory; University of Arizona; Tucson Arizona USA

4. Space and Atmospheric Physics Group, Department of Physics; Imperial College London; London UK

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/ja/ja1111/2011JA016808/2011JA016808.pdf

Reference37 articles.

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2. Simulating the time-dependent response of Titan's upper atmosphere to periods of magnetospheric forcing;Bell;Geophys. Res. Lett.,2011

3. The variability of Titan's magnetic environment;Bertucci;Planet. Space Sci.,2009

4. Planetary coronae and atmospheric evaporation;Chamberlain;Planet. Space Sci.,1963

5. Energetic ion precipitation at Titan;Cravens;Geophys. Res. Lett.,2008

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