Comparing Jupiter’s Equatorial X‐Ray Emissions With Solar X‐Ray Flux Over 19 Years of the Chandra Mission

We present a statistical study of Jupiter’s disk X‐ray emissions using 19 years of Chandra X‐Ray Observatory (CXO) observations. Previous work has suggested that these emissions are consistent with solar X‐rays elastically scattered from Jupiter’s upper atmosphere. We showcase a new pulse invariant...

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Detalles Bibliográficos
Autores principales: 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.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: John Wiley and Sons Inc. 2022
Materias:
Research Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10078327/
https://www.ncbi.nlm.nih.gov/pubmed/37032656
http://dx.doi.org/10.1029/2022JA030971

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10078327/
https://www.ncbi.nlm.nih.gov/pubmed/37032656
http://dx.doi.org/10.1029/2022JA030971

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