Defining Radiation Belt Enhancement Events Based on Probability Distributions
Abstract We present a methodology to define moderate, strong, and intense space weather events based on probability distributions. We have illustrated this methodology using a long‐duration, uniform data set of 1.8–3.5 MeV electron fluxes from multiple LANL geosynchronous satellite instruments, but...
Saved in:
Main Authors: | Geoffrey D. Reeves, Elizabeth M. Vandegriff, Jonathan T. Niehof, Steven K. Morley, Gregory S. Cunningham, Michael G. Henderson, Brian A. Larsen |
---|---|
Format: | Article |
Language: | English |
Published: |
Wiley
2020-08-01
|
Series: | Space Weather |
Subjects: | |
Online Access: | https://doi.org/10.1029/2020SW002528 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Atmospheric Ionizations by Solar X‐Rays, Solar Protons, and Radiation Belt Electrons in September 2017 Space Weather Event
by: Kiyoka Murase, et al.
Published: (2023-12-01) -
Relativistic Electron Model in the Outer Radiation Belt Using a Neural Network Approach
by: Xiangning Chu, et al.
Published: (2021-12-01) -
Forecasting GOES 15 >2 MeV Electron Fluxes From Solar Wind Data and Geomagnetic Indices
by: C. Forsyth, et al.
Published: (2020-08-01) -
Harmonization of RBSP and Arase Energetic Electron Measurements Utilizing ESA Radiation Monitor Data
by: Ingmar Sandberg, et al.
Published: (2021-06-01) -
Relationship Between NM Data and Radiation Dose at Aviation Altitudes During GLE Events
by: N. Larsen, et al.
Published: (2024-06-01)