Figure 1 from HEATING OF THE PARTIALLY IONIZED SOLAR CHROMOSPHERE BY WAVES IN MAGNETIC STRUCTURES

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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 1.

Geometry of the magnetic field. 3D view combining the magnetic field lines (black), location of strong currents (yellow), relative temperature enhancements (﹩+500\;{\rm{K}}﹩, red), and plasma ﹩\beta =1﹩ sufraces (gray) at the simulation time t = 240 s.

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