Image Details

Choose export citation format:

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 3.

Occurrence plots of the perpendicular current ﹩{J}_{\perp }﹩ vs. the amplitude of the magnetic field fluctuation due to the Alfvén wave (left) and the fast wave (right). The magnetic field fluctuations were obtained using the projections of the magnetic field perturbations onto the directions, given by Equations (13)–(15).

Other Images in This Article
Copyright and Terms & Conditions