Journal article
Jovian Auroral Radio Sources Detected In Situ by Juno/Waves: Comparisons With Model Auroral Ovals and Simultaneous HST FUV Images
Geophysical research letters, Vol.46(21), pp.11606-11614
11/16/2019
DOI: 10.1029/2019GL084799
Abstract
Since the discovery of Jovian auroral radio emissions, the question arises of the source positions of the different components (broadband kilometric, hectometric, and decametric) and their association with far ultraviolet (FUV) auroral emissions. We surveyed Juno's first 15 perijoves to track local radio sources from in situ Juno/Waves measurements (50 Hz to 40 MHz). This allowed us to study the 3-D spatial distribution of the broadband kilometric, hectometric, and decametric radio sources. These sources are carried by the same magnetic field lines, with the bulk of them at apex M ranging from 15 to 60 (distance measured in RJ at the magnetic equator). Finally, comparisons with images of the Jovian FUV aurorae simultaneously acquired by the Hubble Space Telescope (HST) reveal a partial spatial colocation of the FUV main oval emission with the identified local radio sources.
Details
- Title: Subtitle
- Jovian Auroral Radio Sources Detected In Situ by Juno/Waves: Comparisons With Model Auroral Ovals and Simultaneous HST FUV Images
- Creators
- C. K. Louis - Institut de Recherche en Astrophysique et PlanétologieR. Prangé - Délégation Paris 7L. Lamy - Délégation Paris 7P. Zarka - Délégation Paris 7M. Imai - University of IowaW. S. Kurth - University of IowaJ. E. P. Connerney - Goddard Space Flight Center
- Resource Type
- Journal article
- Publication Details
- Geophysical research letters, Vol.46(21), pp.11606-11614
- DOI
- 10.1029/2019GL084799
- ISSN
- 0094-8276
- eISSN
- 1944-8007
- Language
- English
- Date published
- 11/16/2019
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9984455272702771
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