Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

The 3He-rich SEP on Event 2024 April 1 at 27 Solar Radii—Indications of Acceleration by Waves and Implications of Coronal Source Location

  • Authors: D. G. Mitchell, D. Lario, N. E. Raouafi, G. M. Mason, A. Kouloumvakos, H. Collier, E. C. Roelof, G. Berland, D. J. McComas, C. M. S. Cohen, M. E. Hill, R. L. McNutt, P. S. Mostafavi, J. C. Kasper, S. D. Bale, M. Pulupa, P. L. Whittlesey

D. G. Mitchell et al 2026 The Astrophysical Journal 1003 .

  • Provider: AAS Journals

Caption: Figure 4.

EPI-Lo species spectra, time-integrated over the event. (a) Spectra expressed in energy per charge (keV q–1), using assumed charge states of 1 for H, 2 for He, 6 for O, and 14 for Fe. While different charge-state assumptions for O and Fe are possible, reasonable variations do not significantly affect the relative appearance. (b) Spectra expressed in energy per nucleon (keV amu–1), which is the conventional representation used in most SEP analyses; we show it here for comparison.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse