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Chromospheric Evaporation via Alfvén Waves

  • Authors: Gerhard Haerendel

HAERENDEL 2009 The Astrophysical Journal 707 903.

  • Provider: AAS Journals

Caption: Figure 8.

View of Poynting flux, S , field-aligned currents, J , loop-top source current, j LT, and driving and transferred forces, F , in a flare loop. The associated distortions of the flux tube are shown by the dashed line contour of the cross section at a midway position.

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