Radiation Belt Model Including Semi‐Annual Variation and Solar Driving (Sentinel)
Abstract The Earth's outer radiation belt response to geospace disturbances is extremely variable spanning from a few hours to several months. In addition, the numerous physical mechanisms, which control this response depend on the electron energy, the timescale, and the various types of geospa...
Saved in:
Main Authors: | C. Katsavrias, S. Aminalragia‐Giamini, C. Papadimitriou, I. A. Daglis, I. Sandberg, P. Jiggens |
---|---|
Format: | Article |
Language: | English |
Published: |
Wiley
2022-01-01
|
Series: | Space Weather |
Subjects: | |
Online Access: | https://doi.org/10.1029/2021SW002936 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
The EMERALD Model for the Estimation of the Radial Diffusion Coefficients in the Outer Belt
by: S. Aminalragia‐Giamini, et al.
Published: (2023-01-01) -
Improving the Electron Radiation Belt Nowcast and Forecast Using the SafeSpace Data Assimilation Modeling Pipeline
by: A. Brunet, et al.
Published: (2023-08-01) -
Strong Relativistic Electron Flux Events in GPS Orbit
by: Nigel P. Meredith, et al.
Published: (2024-12-01) -
Estimation of Geometric Factors for the Particle Detecting Instruments of the Geostationary Satellite GK2A at 128.2°E Longitude Based on Observations of the Outer Radiation Belt During Geomagnetically Quiet Periods
by: W.‐H. Seol, et al.
Published: (2023-01-01) -
Harmonization of RBSP and Arase Energetic Electron Measurements Utilizing ESA Radiation Monitor Data
by: Ingmar Sandberg, et al.
Published: (2021-06-01)