Phase Mixing of Propagating Alfvén Waves in a Single-fluid Partially Ionized Solar Plasma
The phase mixing of Alfvén waves is one of the most promising mechanisms for the heating of the solar atmosphere. The damping of waves in this case requires small transversal scales, relative to the magnetic field direction; this requirement is achieved by considering a transversal inhomogeneity in...
Main Authors: | M. McMurdo, I. Ballai, G. Verth, A. Alharbi, V. Fedun |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2023-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/ad0364 |
Similar Items
-
Persistence of Ion Cyclotron Waves and Stochasticity of Kinetic Alfvén Waves in the Solar Wind
by: Daniele Telloni
Published: (2020-12-01) -
Alfvén Wave Connection between the Chromosphere and the Corona of the Sun: An Analytical Study
by: Jongchul Chae, et al.
Published: (2023-01-01) -
Spectroscopic Detection of Alfvénic Waves in the Chromospheric Fibrils of a Solar-quiet Region
by: Hannah Kwak, et al.
Published: (2023-01-01) -
The Alpha-proton Differential Flow in the Alfvénic Young Solar Wind: from Sub-Alfvénic to Super-Alfvénic
by: Hao Ran, et al.
Published: (2024-01-01) -
Nonlinear Coupling of Alfvén and Slow Magnetoacoustic Waves in Partially Ionized Solar Plasmas: The Effect of Thermal Misbalance
by: José Luis Ballester
Published: (2023-03-01)