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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 1.

Left: the damping time of the standing slow, τslow (blue), and entropy, τentropy (red), modes, obtained from a numerical solution of Equation (5) as a function of temperature for a loop of length L = 180 Mm and plasma density ρ0 = 3 × 10−12 kg m−3. Right: ratio τentropy/τslow from Equation (5) as a function of loop temperature and density (for the same loop length). Contours of τentropy/τslow = 0.3 and 0.1 are shown as red dotted and solid lines, respectively.

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