Identifying the variety of jovian X-ray auroral structures: tying the morphology of X-ray emissions to associated magnetospheric dynamics

Beskrivning

The data used in Weigt et al., study "Identifying the variety of jovian X-ray auroral structures: tying the morphology of X-ray emissions to associated magnetospheric dynamics". The README.pdf explains what data is used to produce each Figure in the article with links to the Chandra archive and other data repositories. Pipeline to analyse data can be found here: https://doi.org/10.5281/zenodo.7380282

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Publiceringsår

2023

Typ av data

Upphovspersoner

Aalto-universitetet

Department of Computer Science

Dale M. Weigt - Upphovsperson

Boston University

Marissa F. Vogt - Upphovsperson

LESIA Space Laboratory

Corentin K. Louis - Upphovsperson

National Institute of Information and Communications Technology

Chihiro Tao - Upphovsperson

School of Cosmic Physics, Dublin Institute for Advanced Studies, Dublin, 2, Ireland

Caitriona M. Jackman - Upphovsperson

Seán McEntee - Upphovsperson

Smithsonian Astrophysical Observatory

Ralph Kraft - Upphovsperson

Southwest Research Institute

Randy Gladstone - Upphovsperson

Space Research Corporation

J. E. P. Connerney - Upphovsperson

UCL

Graziella Branduardi-Raymont - Upphovsperson

William R. Dunn - Upphovsperson

University of Iowa

William S. Kurth - Upphovsperson

University of Lancaster

Diego Moral Pombo - Upphovsperson

Sarah V. Badman - Upphovsperson

University of Liège

Denis Grodent - Upphovsperson

Zenodo - Utgivare

Projekt

Övriga uppgifter

Vetenskapsområden

Data- och informationsvetenskap

Språk

Öppen tillgång

Öppet

Licens

Creative Commons Attribution 4.0 International (CC BY 4.0)

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