MOSWOC high energy electron forecast for geostationary orbit
Forecaster summary - Issued 2021-08-01T00:16:08
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 into the Moderate flux range (100-1000pfu) most likely. Resultant 24-hour integrated fluence showing an upward trend will probably plateau over the next 12 to 24 hours and are comfortably anticipated to remain below the Active threshold.
A similar magnitude reaction is possible towards the end of the forecast period in response to any high speed stream or marginal influence from CH80/- and the 28 July CME. REFM 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 2021-08-01T00:16:08 | ||
| Probability of threshold exceedance | ||
| Active | V.Active | |
| Day 1 | 5% | 1% |
| Day 2 | 10% | 1% |
| Day 3 | 20% | 1% |
| Day 4 | 20% | 1% |