Radio Absorption in the Nightside Ionosphere of Mars During Solar Energetic Particle Events
Abstract Characterization, understanding, and prediction of the Martian radio environment are of increasing importance to the forthcoming human exploration of Mars. Here we investigate 3–5 MHz radio absorption in the nightside ionosphere of Mars caused by enhanced ionization at <100 km altitudes...
Saved in:
Main Authors: | Y. Harada, Y. Nakamura, B. Sánchez‐Cano, M. Lester, N. Terada, F. Leblanc |
---|---|
Format: | Article |
Language: | English |
Published: |
Wiley
2023-12-01
|
Series: | Space Weather |
Subjects: | |
Online Access: | https://doi.org/10.1029/2023SW003755 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Solar Wind With Field Lines and Energetic Particles (SOFIE) Model: Application to Historical Solar Energetic Particle Events
by: Lulu Zhao, et al.
Published: (2024-09-01) -
Towards advanced forecasting of solar energetic particle events with the PARASOL model
by: Afanasiev Alexandr, et al.
Published: (2025-01-01) -
Predicting Solar Energetic Particle Events with Time Series Shapelets
by: Omar Bahri, et al.
Published: (2025-01-01) -
Modeling the transport and anisotropy of energetic electrons in solar flares
by: Xiangliang Kong, et al.
Published: (2025-01-01) -
Delay of Near-relativistic Electrons with Respect to Type III Radio Bursts throughout the Inner Heliosphere
by: J. G. Mitchell, et al.
Published: (2025-01-01)