MOSWOC high energy electron forecast for geostationary orbit
Forecaster summary - Issued 2020-02-28T00:04:47
The high energy electron flux (greater than 2MeV) is likely to continue its current behaviour of mainly Moderate flux (100-1000pfu) in the near-term. The probabilities of this shifting to High diurnal peaks should increase in the second half of the four-day period, as a result of potentially becoming affected by CH18 and any northward extension of the southern polar coronal hole.
Both the REFM forecast and 27-day recurrence suggest the fluence should remain below the Active threshold. Typical probabilities are given as 10 to 15 percent by the Recurrence-Persistence model for Days 2 to 4. The preferred forecast is for a more reactive increase over the same period: i.e. initially lower, and later marginally higher probabilities than these models suggest into the new week, due to the possibility of a weak connection between CH18 and the southern crown, and Earth's being slightly further south (relative to the solar equator) this pass.
| High Energy Electron Event Forecast | ||
|---|---|---|
| Issued 2020-02-28T00:04:47 | ||
| Probability of threshold exceedance | ||
| Active | V.Active | |
| Day 1 | 1% | 1% |
| Day 2 | 5% | 1% |
| Day 3 | 20% | 1% |
| Day 4 | 20% | 1% |