Image Details

Choose export citation format:

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 4.

Carrington longitude of Solar Orbiter photospheric footpoints versus time. Solid curves show SO, SO−10, and SO+10. Dashed curves SO−sw and SO+sw show the longitude uncertainty from measured vsw variability during the injection (03:00–05:00 UT) and dropout (07:00–10:00 UT) intervals. The × symbols mark photospheric footpoints of open-to-ecliptic field lines (∣λSS∣≤7°), colored by polarity (green for positive, red for negative). Photospheric footpoints whose source-surface endpoints lie at other latitudes (shown in Figure 3) are omitted for clarity. The gray band denotes the EUV jet-base longitude range.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse