SIMULATION OF FAST MAGNETOACOUSTIC WAVES IN THE SOLAR CORONAL MAGNETIC STRUCTURES
MHD waves in force-free magnetic arcades describing bipolar solar active regions are studied. The geometric acoustics approximation is used in cases where the wavelength is small compared to the scale of the inhomogeneity. It allows simple mathematical models to study phenomena such as wave refracti...
Saved in:
Main Authors: | B. B. Mikhalyaev, G. A. Mankaeva, L. N. Dzhimbeeva, O. V. Hongorova, S. B. Derteev |
---|---|
Format: | Article |
Language: | Russian |
Published: |
North-Caucasus Federal University
2022-08-01
|
Series: | Современная наука и инновации |
Subjects: | |
Online Access: | https://msi.elpub.ru/jour/article/view/252 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Project Sun Gazers
by: O. N. Mikhalyaev, et al.
Published: (2024-03-01) -
Quantifying Suppression of Solar Surface Magnetic Flux Advection with Increasing Field Strength
by: V. Aparna, et al.
Published: (2025-01-01) -
Steady-state Heating of Diffuse Coronal Plasma in a Solar Active Region
by: Gregory D. Fleishman, et al.
Published: (2025-01-01) -
P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona
by: Supriya Hebbur Dayananda, et al.
Published: (2025-01-01) -
Understanding the Complex Morphology of a Coronal Mass Ejection: Multiview Analysis and Numerical Modeling
by: Cecilia Mac Cormack, et al.
Published: (2025-01-01)