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Charge States of Energetic Solar Ions from Coronal Shock Acceleration

  • Authors: Marianna Lytova and Leon Kocharov

Lytova & Kocharov 2005 The Astrophysical Journal Letters 620 L55.

  • Provider: AAS Journals

Caption: Fig. 1.

Mean charge states of Fe in shock‐accelerated particles escaping into the interplanetary medium. The particle escape is dominated either by diffusion (D: model 1; histogram) or by convection (C: model 2; plus signs, diamonds, and circles). The normalization coefficient of the coronal density profile is shown in parentheses (eq. [2]).

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