Determining the Beaming of Io Decametric Emissions: A Remote Diagnostic to Probe the Io‐Jupiter Interaction-Reference-Cited by-同舟云学术

Determining the Beaming of Io Decametric Emissions: A Remote Diagnostic to Probe the Io‐Jupiter Interaction

Published:2022-04 Issue:4 Volume:127 Page:
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:JGR Space Physics

Author:

Lamy L.¹²³^ORCID,Colomban L.⁴^ORCID,Zarka P.¹²^ORCID,Prangé R.¹,Marques M. S.⁵,Louis C. K.⁶^ORCID,Kurth W. S.⁷^ORCID,Cecconi B.¹²^ORCID,Girard J. N.¹^ORCID,Grießmeier J.‐M.²⁴^ORCID,Yerin S.⁸⁹^ORCID

Affiliation:

1. LESIA Observatoire de Paris Université PSL CNRS Sorbonne Université Université Paris Cité Meudon France

2. Station de Radioastronomie de Nancay Observatoire de Paris Université PSL CNRS University Orléans Nancay France

3. Aix Marseille Université CNRS CNES LAM Marseille France

4. LPC2E CNRS Université d’Orléans Orléans France

5. Departamento de Geofisica Universidade Federal do Rio Grande do Norte Natal Brazil

6. School of Cosmic Physics DIAS Dusink Observatory, Dublin Institute for Adanced Studies Dublin Ireland

7. Department of Physics and Astronomy University of Iowa Iowa IA USA

8. Institute of Radio Astronomy of NAS of Ukraine Kharkiv Ukraine

9. V. N. Karazin Kharkiv National University Kharkiv Ukraine

Funder

Centre National d’Etudes Spatiales

Institut national des sciences de l'Univers

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2021JA030160

Reference51 articles.

1. Auroral Processes at the Giant Planets: Energy Deposition, Emission Mechanisms, Morphology and Spectra

2. Influence of the Satellite Io on Jupiter's Decametric Emission

3. A new high-grain, broadband, steerable array to study Jovian decametric emission

4. The Io UV footprint: Location, inter-spot distances and tail vertical extent

5. UV Io footprint leading spot: A key feature for understanding the UV Io footprint multiplicity?

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