Emesso: 2017 Dec 03 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Moderate (ISES: Major) magstorm expected (A>=50 or K=6)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 03 Dec 2017 | 071 | 004 |
| 04 Dec 2017 | 070 | 054 |
| 05 Dec 2017 | 070 | 045 |
Solar activity was at very low levels. The Sun is spotless. No earth-directed coronal mass ejections (CMEs) were observed in available coronagraphic imagery. The greater than 10 MeV proton flux was at nominal levels.
Quiet flaring conditions are expected.
ACE data indicated solar wind speed decreased further from initial values near 400 km/s to about 350 km/s by the end of the period. Bz varied between +3 nT and -4 nT. The interplanetary magnetic field was mostly directed towards the Sun. The extension of a positive northern polar CH is transiting the central meridian.
The geomagnetic field was quiet to unsettled levels throughout the period, and is expected to remain so until the arrival of the high speed stream from the northern polar coronal hole (CH) extension and its associated preceding co-rotating interaction region. Based on observations from the previous solar rotation and from STEREO-A, their influence may start affecting the earth environment late on 03 December or on 04 December, with minor to moderate geomagnetic storming possible.
Today's estimated international sunspot number (ISN): 000, based on 09 stations.
| Wolf number Catania | /// |
| 10cm solar flux | 072 |
| AK Chambon La Forêt | 006 |
| AK Wingst | 003 |
| Estimated Ap | 003 |
| Estimated international sunspot number | 000 - Based on 13 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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