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Solar Orbiter Solar Energetic Particle Dropout during a Magnetic Cloud with Evidence for Strong Connectivity Gradients

  • Authors: Radoslav Bučík, Raúl Gómez-Herrero, Samuel T. Hart, Maher A. Dayeh, Nariaki V. Nitta

Radoslav Bučík et al 2026 The Astrophysical Journal Letters 1006 .

  • Provider: AAS Journals

Caption: Figure 2.

SDO image of the solar source at time of the event-associated type III radio burst. AIA 171 Å is shown in green and the HMI line-of-sight magnetic field (scaled to ±150 G) in black and red tinted colors. Jet is marked by arrow; a 5° Carrington grid is overlaid. The × symbols mark photospheric footpoints of field lines open to the ecliptic, and the + symbols mark footpoints of field lines open to other latitudes at the source surface (Section 5).

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