Mapping the Brightness of Ganymede's Ultraviolet Aurora Using Hubble Space Telescope Observations
We analyze Hubble Space Telescope observations of Ganymede made with the Space Telescope Imaging Spectrograph between 1998 and 2017 to generate a brightness map of Ganymede's oxygen emission at 1,356 Å. Our Mercator projected map demonstrates that the brightness along Ganymede's northern a...
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Bibliographic Details
Published in: | Journal of Geophysical Research: Planets |
Main Authors: |
Marzok, A.,
Schlegel, S.,
Saur, J.,
Roth, L.,
Grodent, D.,
Strobel, D. F.,
Retherford, K. D.,
Marzok, A.; 1 Institute of Geophysics and Meteorology, University of Cologne Cologne Germany,
Schlegel, S.; 1 Institute of Geophysics and Meteorology, University of Cologne Cologne Germany,
Roth, L.; 2 School of Electrical Engineering, KTH Royal Institute of Technology Stockholm Sweden,
Grodent, D.; 3 Laboratoire de Physique Atmosphérique et Planétaire, STAR Institute, University of Liège Liège Belgium,
Strobel, D. F.; 4 Department of Earth and Planetary Science, and Department of Physics and Astronomy, The Johns Hopkins University Baltimore MD USA,
Retherford, K. D.; 5 Southwest Research Institute San Antonio TX USA |
Format: | Article in Journal/Newspaper
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Language: | English |
Published: |
2022
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Subjects: |
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Online Access: | https://doi.org/10.1029/2022JE007256
http://resolver.sub.uni-goettingen.de/purl?gldocs-11858/10249
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