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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. 2.

Mean charge states of Fe in particles escaping into the interplanetary medium (diamonds), in particles registered near the shock (plus signs), and in particles far downstream from the shock (histogram). The symbols correspond to model 2. The histogram is for the particle escape at a fixed distance (104 km) downstream from the shock. In Figs. 24, the density normalization is nominal (﹩\rho =1﹩).

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