Emesso: 2018 Sep 09 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Minor storm expected (A>=30 or K=5)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 09 Sep 2018 | 069 | 008 |
| 10 Sep 2018 | 069 | 013 |
| 11 Sep 2018 | 069 | 034 |
Solar activity was at very low levels. Small and inactive sunspot region NOAA 2721 is still present on the solar disk. 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 trans-equatorial positive polarity coronal hole (CH) has finished its transit over the Central Meridian.
Solar activity is expected to remain at very low levels.
Solar wind speed varied between 360 and 430 km/s, ending the period near 370 km/s (DSCOVR). Bz varied mostly between -4 and +3 nT, ending the period at +6 nT. The direction of the interplanetary magnetic field was variable.
Quiet to unsettled geomagnetic conditions were observed. Mostly quiet geomagnetic conditions are expected with a chance on an unsettled episode until the arrival of the co-rotating interaction region (CIR) and wind stream from the positive polarity CH, late on 10 or on 11 September. This may result in minor storming conditions.
Today's estimated international sunspot number (ISN): 015, based on 21 stations.
| Wolf number Catania | /// |
| 10cm solar flux | 069 |
| AK Chambon La Forêt | 009 |
| AK Wingst | 005 |
| Estimated Ap | 005 |
| Estimated international sunspot number | 016 - Based on 23 stations |
| Day | Begin | Max | Fine | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
|---|---|---|---|---|---|---|---|---|---|---|
| Nessuna | ||||||||||
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
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