Issued: 2019 Sep 30 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
30 Sep 2019 | 067 | 019 |
01 Oct 2019 | 067 | 016 |
02 Oct 2019 | 067 | 011 |
Solar activity was at very low levels. The Sun was spotless again. No earth-directed coronal mass ejections (CMEs) have been observed in available coronagraphic imagery. The greater than 10 MeV proton flux was at nominal values.
Solar activity is expected to remain at very low levels.
Solar wind speed declined from initial values around 530 km/s to 440 km/s at the end of the period (ACE). Bz was weakly but almost continuously negative with sustained values near -5 nT. These solar wind conditions resulted in some active geomagnetic intervals in both Kp and K Dourbes. The interplanetary magnetic field (phi angle) was mostly directed away from the Sun (positive sector).
Geomagnetic activity is expected to be mostly at quiet to unsettled levels, as the Earth remains under the gradually weakening influence from the coronal hole wind stream. There remains a chance on an active episode.
Today's estimated international sunspot number (ISN): 000, based on 25 stations.
Wolf number Catania | /// |
10cm solar flux | 067 |
AK Chambon La Forêt | 030 |
AK Wingst | 014 |
Estimated Ap | 016 |
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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