Issued: 2019 Sep 29 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 29 Sep 2019 | 068 | 018 |
| 30 Sep 2019 | 068 | 010 |
| 01 Oct 2019 | 068 | 005 |
Solar X-ray flux remained below B class levels throughout the period. The Solar disk is spotless and the X-ray flux is expected to remain at or below background levels.
There were no Earth-directed Coronal Mass Ejections (CME) observed in coronagraph data.
Proton levels were at background values and are expected to remain so.
The solar wind speed has decreased from 650 and 540 km/s over the past 24 hours. The total magnetic field strength has fluctuated around 5 nT. The Bz ranged between -4 and 4 nT. Geomagnetic conditions ranged between Kp index 2-5 (NOAA) and local K index 1-4 (Dourbes).
The enhanced solar wind conditions experienced are from a high speed stream (HSS) from a recurrent positive polarity coronal hole. The solar wind speeds are now starting to abate and should return to nominal levels in a couple of days.
Geomagnetic conditions are expected to be unsettled, with some active periods due to HSS solar wind enhancements.
Today's estimated international sunspot number (ISN): 000, based on 11 stations.
| Wolf number Catania | /// |
| 10cm solar flux | 067 |
| AK Chambon La Forêt | 029 |
| AK Wingst | 027 |
| Estimated Ap | 030 |
| Estimated international sunspot number | 000 - Based on 26 stations |
| Day | Begin | Max | End | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
|---|---|---|---|---|---|---|---|---|---|---|
| None | ||||||||||
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
All times in UTC
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