MOSWOC high energy electron forecast for geostationary orbit
Forecaster summary - Issued 2021-07-30T00:18:13
High energy electron flux (greater than 2MeV) has recently shown an upward trend in reaction to the high speed stream from coronal hole 78/79/+. While this response may not yet have stabilised, in all likelihood further increases should be limited, with diurnal peaks in the Moderate flux range (100-1000pfu) most likely. Resultant 24-hour integrated fleunce should show an upward trend, but will probably soon plateau and should consequently fall comfortably short of Active.
A similar magnitude reaction is possible to end the four days in response to any high speed stream or marginal CME influence from CH80/- and the 28 July CME. The presence of two transients in the forecast limits the usefulness of REFM in the period, however its suggestion of sub-Active fluence is felt to be accurate should the ambient or coronal hole-driven wind continue throughout.
| High Energy Electron Event Forecast | ||
|---|---|---|
| Issued 2021-07-30T00:18:13 | ||
| Probability of threshold exceedance | ||
| Active | V.Active | |
| Day 1 | 5% | 1% |
| Day 2 | 10% | 1% |
| Day 3 | 5% | 1% |
| Day 4 | 20% | 1% |