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Chromospheric Evaporation via Alfvén Waves

  • Authors: Gerhard Haerendel

HAERENDEL 2009 The Astrophysical Journal 707 903.

  • Provider: AAS Journals

Caption: Figure 6.

(a) Cartoon of the loop-top plasma layer arising from braking of the reconnection jet, possibly by fast shock formation. (b) One flare loop out of an arcade (top left) guides energy toward the highly structured chromosphere via an Alfvén wave, which is launched by the grad- B currents.

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