Figure 4 from Tuning the Exospace Weather Radio for Stellar Coronal Mass Ejections

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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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