Issued: 2018 Dec 11 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 11 Dec 2018 | 071 | 010 |
| 12 Dec 2018 | 070 | 012 |
| 13 Dec 2018 | 069 | 007 |
Solar activity has been quiet over the past 24 hours. There are no significant Active Regions on the solar disk. Flaring conditions are expected to remain quiet with a very small change of C-class flares.
No Earth directed Coronal Mass Ejection have been observed. The greater than 10 MeV solar protons flux remained at background levels over the past 24 hours and are expected to remain so.
The solar wind speed has been slowly decreasing from around 650 to 525 km/s over the past 24 hours. The total magnetic field strength has fluctuated around 5 nT. The Bz component was largely positive, fluctuating between -5 and +5 nT.
The elevated solar wind speeds were a consequence of a large Coronal Hole (which reached the central meridian on December 04). The enhanced solar wind conditions are beginning to abate but could still cause enhanced geomagnetic activity.
Geomagnetic conditions ranged between Kp index 1-3 (NOAA) and local K index 1-3 (Dourbes) over the past 24 hours.
Today's estimated international sunspot number (ISN): 012, based on 16 stations.
| Wolf number Catania | 000 |
| 10cm solar flux | 071 |
| AK Chambon La Forêt | 013 |
| AK Wingst | /// |
| Estimated Ap | 011 |
| 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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