Flux Rope Eruption From the Sun to the Earth: What do Reversals in the Azimuthal Magnetic Field Gradient Tell us About the Evolution of the Magnetic Structure?

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ADS bibcode
2008AGUFMSH23B1638S
year
2008
Listed Authors
Steed, K.
Owen, C. J.
Harra, L. K.
Green, L. M.
Dasso, S.
Walsh, A. P.
Démoulin, P.
van Driel-Gesztelyi, L.
Listed Institutions
UCL - Mullard Space Science Laboratory, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, United Kingdom
UCL - Mullard Space Science Laboratory, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, United Kingdom
UCL - Mullard Space Science Laboratory, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, United Kingdom
UCL - Mullard Space Science Laboratory, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, United Kingdom
Universidad de Buenos Aires, Departmento de Física (FCEN-UBA) and Instituto de Astronomía y Física del Espacio, CONICET-UBA, CC. 67, Suc. 28, Buenos Aires, 1428, Argentina
UCL - Mullard Space Science Laboratory, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, United Kingdom
Observatoire de Paris, LESIA, UMR 8109 (CNRS), Meudon, 92195, France
Observatoire de Paris, LESIA, UMR 8109 (CNRS), Meudon, 92195, France; UCL - Mullard Space Science Laboratory, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, United Kingdom

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