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HEATING OF THE PARTIALLY IONIZED SOLAR CHROMOSPHERE BY WAVES IN MAGNETIC STRUCTURES

  • Authors: S. Shelyag, E. Khomenko, A. de Vicente, and D. Przybylski

2016 The Astrophysical Journal Letters 819 L11.

  • Provider: AAS Journals

Caption: Figure 5.

Poynting flux absorption. Left panel: height dependence of temporally and horizontally averaged Poynting flux for the W simulation (FW, red curve) and for the ADW simulation with the wave source and ambipolar diffusion term (FADW, black curve). Right panel: dependence of Poynting flux absorption ﹩1-{F}_{{ADW}}/{F}_{W}﹩ on height in the simulation.

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