Image Details

Choose export citation format:

Entropy-mode Imprints in the Solar Corona: Nonexponential Damping and Phase Shifts of Compressive Oscillations

  • Authors: Dmitrii Kolotkov, Sergey Belov, Mohamed Sherif

Dmitrii Kolotkov et al 2026 The Astrophysical Journal Letters 1004 .

  • Provider: AAS Journals

Caption: Figure 4.

Left: spatiotemporal evolution of the fundamental harmonic of the slow mode (red circles), entropy mode (blue squares), and full numerical solution of Equations (1)–(4) (gray dashed) for loop temperature perturbation. The time dependence of the slow and entropy modes is given by Equations (13) and (14); the spatial structure of their amplitudes AT,slow(z) and AT,entropy(z) is obtained as described in Section 3.3. Right: same as left column but for plasma density perturbations.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse