Spectral morphology of the X-ray emission from Jupiter's aurorae

Author:

Branduardi-Raymont G.1,Elsner R. F.2,Galand M.3,Grodent D.4,Cravens T. E.5,Ford P.6,Gladstone G. R.7,Waite J. H.7

Affiliation:

1. Mullard Space Science Laboratory; University College London; Holmbury St. Mary UK

2. NASA Marshall Space Flight Center; NSSTC/XD12, Space Science Branch; Huntsville Alabama USA

3. Imperial College London, Space and Atmospheric Physics Group; Blackett Laboratory; London UK

4. Laboratoire de Physique Atmosphérique et Planétaire, Institut d'Astrophysique et de Géophysique; Université de Liège; Liège Belgium

5. Department of Physics and Astronomy; University of Kansas; Lawrence Kansas USA

6. Massachusetts Institute of Technology; Kavli Institute for Astrophysics and Space Research; Cambridge Massachusetts USA

7. Southwest Research Institute; San Antonio Texas 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

Reference22 articles.

1. Auroral emissions of the giant planets;Bhardwaj;Rev. Geophys.,2000

2. Low- to middle-latitude X-ray emission from Jupiter;Bhardwaj;J. Geophys. Res.,2006

3. X-rays from solar system bodies;Bhardwaj;Planet. Space Sci.,2007

4. First observation of Jupiter by XMM-Newton;Branduardi-Raymont;Astron. Astrophys.,2004

5. A study of Jupiter's aurorae with XMM-Newton;Branduardi-Raymont;Astron. Astrophys.,2007

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