Issued: 2013 Mar 17 1136 UTC
Eruptive (C-class flares expected, probability >= 50%)
Minor geomagnetic storm expected (A>=30 or K=5)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 17 Mar 2013 | 126 | 026 |
| 18 Mar 2013 | 124 | 004 |
| 19 Mar 2013 | 123 | 004 |
Solar activity has been quiet, but is expected to be eruptive for the next 24 hours. The full halo CME of Friday March 15th has arrived since Sunday March 17th around 6 o'clock and geomagnetic activity has reached storm levels since 9:00 UT. The Solar wind speed jumped to around 700 km/s. The interplanetary magnetic field Bz component is turbulent around -15 nT. Active to Storm geomagnetic conditions are expected for the next few hours, but will return to quiet levels after that. Proton levels of 10 MeV are dropping below the 10 pfu treshold again.
Today's estimated international sunspot number (ISN): 073, based on 06 stations.
| Wolf number Catania | /// |
| 10cm solar flux | 126 |
| AK Chambon La Forêt | 013 |
| AK Wingst | 012 |
| Estimated Ap | 012 |
| Estimated international sunspot number | 077 - Based on 11 stations |
| Day | Begin | Max | End | Loc | Strength | OP | 10cm | Radio burst types | Catania/NOAA | |
|---|---|---|---|---|---|---|---|---|---|---|
| None | ||||||||||
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
All times in UTC
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