Evolution of Alfvén Waves in the Solar Wind. II. Broadband Driver

The propagation of azimuthal Alfvén waves and their interaction with the solar wind are investigated using a 2.5D magnetohydrodynamic model that incorporates the effects of optically thin radiation, as well as collisional and collisionless thermal conduction. The background plasma forms a dipole fie...

Full description

Saved in:
Bibliographic Details
Main Authors: Khaled Alielden, Yeghiazar Taroyan
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/adc8a0
Tags: Add Tag
No Tags, Be the first to tag this record!