2 papers
astro-ph.SR2025
Self-Consistent Heating of the Magnetically Closed Solar Corona: Generation of Nanoflares, Thermodynamic Response of the Plasma and Observational Signatures
Craig D. Johnston, Lars K. S. Daldorff, James A. Klimchuk +5
The energy that heats the magnetically closed solar corona originates in the complex motions of the massive photosphere. Turbulent photospheric convection slowly displaces the foot…
astro-ph.SR2025
Wave Particle Interaction in the Upstream of ICME Shocks
Shanwlee Sow Mondal, Aveek Sarkar, Sofiane Bourouaine
Shocks associated with Interplanetary Coronal Mass Ejections are known to energize charged particles and give rise to Solar Energetic Particles. Many of these energetic particles m…