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Tuning the Exospace Weather Radio for Stellar Coronal Mass Ejections

  • Authors: Julián D. Alvarado-Gómez, Jeremy J. Drake, Federico Fraschetti, Cecilia Garraffo, Ofer Cohen, Christian Vocks, Katja Poppenhäger, Sofia P. Moschou, Rakesh K. Yadav, and Ward B. Manchester IV

2020 The Astrophysical Journal 895 47.

  • Provider: AAS Journals

Caption: Figure 4.

Snapshot during the temporal evolution of the partially confined CME (﹩{E}_{{\rm{B}},2}^{\mathrm{FR}}\simeq 2.0\times {10}^{35}﹩ erg, ﹩{E}_{{\rm{K}},2}^{\mathrm{CME}}\simeq 3.2\times {10}^{31}﹩ erg, ﹩{M}_{2}^{\mathrm{CME}}\simeq 4.0\times {10}^{15}﹩ g) within our M-dwarf simulation. See the caption of Figure 3. Note the difference in field of view (45 R) and timestamp (50 minutes) in this case.

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