Image Details

Choose export citation format:

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 1.

Meridional projection of the Alfvén speed (VA) in our AWSoM steady-state simulations. Top: Sun (CR 2107). Middle: young Sun-like star (CR 2107 + 75 G large-scale dipole). Bottom: M-dwarf (Proxima Centauri). The sphere represents the stellar surface, color-coded by the radial field (BR) driving each model. The color scaling for VA is preserved in all cases. The VA profiles in Figure 2 have been extracted along the white lines The field of view is 12 R, with a set of selected magnetic field lines in black.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse