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Resolving Compositional Features of Solar Wind Source Regions near the Heliospheric Current Sheet at 0.3 au

  • Authors: Keiichi Ogasawara, 笠原桂一 小, Ryan M. Dewey, Frédéric Allegrini, B. L. Alterman, Antoinette Galvin, Timothy S. Horbury, Lynn Kistler, Susan T. Lepri, Stefano A. Livi, Philippe Louarn, Christopher J. Owen, James M. Raines, Sarah A. Spitzer

Keiichi Ogasawara et al 2026 The Astrophysical Journal 1008 .

  • Provider: AAS Journals

Caption: Figure 1.

(a) Schematic diagram showing locations of the Earth and Solar Orbiter in the solar ecliptic coordinate system during the HCS crossing focused on in this paper. (b) ADAPT magnetogram for the Carrington rotation 2269 with spacecraft footprints and estimated HCS. The coronal holes are also marked with red (blue) for positive (negative) Br. The subspacecraft locations before (blue) and after (red) 6 hr of HCS crossings are marked by the crosses with the magnetic footprints with circles. The expected HCS location is also indicated by the black line. The magnetic footprints are calculated by the magnetic connectivity tool. The green triangles denote locations of active regions identified in CR2269.

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