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Comparing Jupiter's Equatorial X-Ray Emissions With Solar X-Ray Flux Over 19 Years of the Chandra Mission.
McEntee, S C; Jackman, C M; Weigt, D M; Dunn, W R; Kashyap, V; Kraft, R; Louis, C K; Branduardi-Raymont, G; Gladstone, G R; Gallagher, P T.
Afiliação
  • McEntee SC; School of Cosmic Physics DIAS Dunsink Observatory Dublin Institute for Advanced Studies Dublin Ireland.
  • Jackman CM; School of Physics Trinity College Dublin Dublin Ireland.
  • Weigt DM; School of Cosmic Physics DIAS Dunsink Observatory Dublin Institute for Advanced Studies Dublin Ireland.
  • Dunn WR; School of Cosmic Physics DIAS Dunsink Observatory Dublin Institute for Advanced Studies Dublin Ireland.
  • Kashyap V; Department of Physics and Astronomy University College London London UK.
  • Kraft R; Centre for Planetary Sciences at UCL/Birkbeck London UK.
  • Louis CK; Harvard-Smithsonian Center for Astrophysics Smithsonian Astrophysical Observatory Cambridge MA USA.
  • Branduardi-Raymont G; Harvard-Smithsonian Center for Astrophysics Smithsonian Astrophysical Observatory Cambridge MA USA.
  • Gladstone GR; School of Cosmic Physics DIAS Dunsink Observatory Dublin Institute for Advanced Studies Dublin Ireland.
  • Gallagher PT; Mullard Space Science Laboratory Department of Space and Climate Physics University College London Dorking UK.
J Geophys Res Space Phys ; 127(12): e2022JA030971, 2022 Dec.
Article em En | MEDLINE | ID: mdl-37032656
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Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: J Geophys Res Space Phys Ano de publicação: 2022 Tipo de documento: Article
Texto completo
Imprimir
XML
PubMed Links
Buscar no Google

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: J Geophys Res Space Phys Ano de publicação: 2022 Tipo de documento: Article