Frequency Characteristics of Magnetosonic Waves Driven by Hot Ring-Beam Protons
Magnetosonic (MS) waves can be generated by energetic ring-beam protons, appearing as harmonics near the local proton cyclotron frequency, in the planetary ionospheres/magnetospheres. A theoretical dispersion relation is derived using kinetic theory to study the growth and frequency characteristics...
Saved in:
| Main Authors: | Amrutha, S. V. Singh, K. C. Barik, G. S. Lakhina |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
|
| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/adee90 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Magnetosonic Waves Driven by Maxwellian Ring Protons in the Martian Upper Ionosphere
by: Amrutha, et al.
Published: (2025-03-01) -
Solar Wind Control of the Martian Magnetotail Current Sheet and Magnetic Reconnection
by: Lei Wang, et al.
Published: (2025-01-01) -
Effects of the 2018 Martian Global Dust Storm on Boundary Positions in the Induced Magnetosphere
by: Catherine E. Regan, et al.
Published: (2025-01-01) -
Foreshock Ultralow Frequency Waves at Mars: Consequence on the Particle Acceleration Mechanisms at the Martian Bow Shock
by: Nahuel Andrés, et al.
Published: (2025-01-01) -
Multipoint Observations of Magnetic Reconnection in the Martian Magnetotail Triggered by an Interplanetary Magnetic Field Rotation
by: Yuanzheng Wen, et al.
Published: (2025-01-01)