2 papers
astro-ph.SR2026
A Self-consistent Model for the Generation of Coronal Condensations: The Effects of Turbulent Wave Dissipation
M. McMurdo, V. Jercic, T. Van Doorsselaere +1
Prominences and coronal rain are two manifestations of coronal condensations whose formation mechanisms remain only partially understood. While previous studies have explored how l…
astro-ph.SR2025
Uniturbulence and Alfvén Wave Solar Model in MPI-AMRVAC
M. McMurdo, T. Van Doorsselaere, N. Magyar +2
The coronal heating problem remains a fundamental challenge in solar physics. While AWSoM-type models (Alfvén Wave Solar Model) have proven highly successful in reproducing the lar…