Välja antud: 2018 Sep 06 1445 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
06 Sep 2018 | 067 | 009 |
07 Sep 2018 | 068 | 015 |
08 Sep 2018 | 068 | 010 |
Solar activity was at very low levels. The Sun was spotless again. No earth-directed coronal mass ejections (CMEs) were observed in the available coronagraphic imagery. The greater than 10 MeV proton flux was at nominal levels. A positive polarity coronal hole (CH) is approaching the Central Meridian.
Solar activity is expected to remain at very low levels.
Solar wind speed increased from an initial 490 km/s to a maximum of about 510 km/s around 13UT, before gradually declining to its current values just above 400 km/s (DSCOVR). Bz softened from -6 nT at the beginning of the period to a more stable range between -3 and +2 nT after 18UT. The direction of the interplanetary magnetic field was mostly in a positive sector (away from the Sun), with some negative excursions.
Quiet to unsettled geomagnetic conditions were observed, with K Dourbes recording an isolated active episode during the 10-13UT interval on 5 September. Quiet to active geomagnetic conditions are expected in response to the arrival later today or tomorrow (7 September) of the co-rotating interaction region (CIR) and wind stream from the negative polarity CH. A minor storming episode is not excluded.
Today's estimated international sunspot number (ISN): 000, based on 21 stations.
Wolf number Catania | 000 |
10cm solar flux | 068 |
AK Chambon La Forêt | 014 |
AK Wingst | 014 |
Estimated Ap | 014 |
Estimated international sunspot number | 000 - Based on 30 stations |
Day | Begin | Max | Lõpp | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
---|---|---|---|---|---|---|---|---|---|---|
Puuduvad |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
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