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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S327(12), p. 67-70

DOI: 10.1017/s1743921317001077

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Photospheric magnetic field of an eroded-by-solar-wind coronal mass ejection

Journal article published in 2016 by J. Palacios ORCID, C. Cid, E. Saiz, A. Guerrero
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractWe have investigated the case of a coronal mass ejection that was eroded by the fast wind of a coronal hole in the interplanetary medium. When a solar ejection takes place close to a coronal hole, the flux rope magnetic topology of the coronal mass ejection (CME) may become misshapen at 1 AU as a result of the interaction. Detailed analysis of this event reveals erosion of the interplanetary coronal mass ejection (ICME) magnetic field. In this communication, we study the photospheric magnetic roots of the coronal hole and the coronal mass ejection area with HMI/SDO magnetograms to define their magnetic characteristics.