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Energy Transport and Heating by Nonthermal Electrons in a Turbulent Solar Flare Environment

  • Authors: A. Gordon Emslie, Eduard P. Kontar

A. Gordon Emslie and Eduard P. Kontar 2026 The Astrophysical Journal 1001 .

  • Provider: AAS Journals

Caption: Figure 3.

Ohmic heating rate Qrc versus distance from the (loop-top) acceleration region. The solid line shows the results for collisional scattering, and the other lines show the results for turbulent scattering, with a turbulent scattering length λT equal to 0.1× (red), 0.2× (green), and 0.3× (blue) the collisional mean free path of 7 × 107 cm. (Note that the abscissa is now on a logarithmic scale).

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