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LONGITUDINAL PROPERTIES OF A WIDESPREAD SOLAR ENERGETIC PARTICLE EVENT ON 2014 FEBRUARY 25: EVOLUTION OF THE ASSOCIATED CME SHOCK

  • Authors: D. Lario, R.-Y. Kwon, A. Vourlidas, N. E. Raouafi, D. K. Haggerty, G. C. Ho, B. J. Anderson, A. Papaioannou, R. Gómez-Herrero, N. Dresing, and P. Riley

2016 The Astrophysical Journal 819 72.

  • Provider: AAS Journals

Caption: Figure 2.

(a)–(b) Coronal magnetic field configuration as seen from Earth on 2014 February 25 at 00:04 UT obtained by (a) the PFSS model and (b) the MAS model. A selection of closed (white) and open (purple) field lines are shown. The black patches on the solar surface (at 1 R) in panel (b) show the location of coronal holes. (c) Combination of images taken by the SOHO/LASCO/C2 and C3 coronagraphs showing the structure of streamers and the presence of a southwestward directed CME (indicated by the arrow) prior to the occurrence of the SEP event on 2014 February 25.

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