Variation of different components of Jupiter's auroral emission-Reference-Cited by-同舟云学术

Variation of different components of Jupiter's auroral emission

Published:2009-06 Issue:A6 Volume:114 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:

Nichols J. D.¹²,Clarke J. T.¹,Gérard J. C.³,Grodent D.³,Hansen K. C.⁴

Affiliation:

1. Center for Space Physics; Boston University; Boston Massachusetts USA

2. Department of Physics and Astronomy; University of Leicester; Leicester UK

3. Laboratory for Planetary and Atmospheric Physics; Institut d'Astrophysique et de Géophysique, Université de Liège; Liege Belgium

4. Department of Atmospheric, Oceanic and Space Sciences; University of Michigan; Ann Arbor Michigan USA

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

Reference43 articles.

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2. Time-resolved observations of Jupiter's far-ultraviolet aurora;Ballester;Science,1996

3. UV Io footprint leading spot: A key feature for understanding the UV Io footprint multiplicity?;Bonfond;Geophys. Res. Lett.,2008

4. Effect of solar wind pressure pulses on the size and strength of the auroral oval;Boudouridis;J. Geophys. Res.,2003

5. Jovian cusp processes: Implications for the polar aurora;Bunce;J. Geophys. Res.,2004

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