Emesso: 2013 Mar 18 1159 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Proton event expected (10 pfu at >10 MeV)
10cm flux | Ap | |
---|---|---|
18 Mar 2013 | 126 | 016 |
19 Mar 2013 | 123 | 006 |
20 Mar 2013 | 123 | 004 |
Solar activity is eruptive with 6 C-flares in the past 12 hours. Four C-flares originated from NOAA AR1698 and two C-flares came from an unnumbered region near AR1700. Solar activity is expected to remain eruptive for the next 24 hours, mainly caused by AR1698. C-flares are very likely, but there is also a slight chance for an M-flare. AR1698 is approaching the west limb, so if it erupts a proton event is possible. The solar wind is getting stable again; in the past 24 hours the speed has decreased from 750 km/s to about 500 km/s. The interplanetary magnetic field has returned to about 10nT, with a positive Bz-component. Geomagnetic conditions are expected to be quiet for the next 48 hours.
Today's estimated international sunspot number (ISN): 069, based on 08 stations.
Wolf number Catania | /// |
10cm solar flux | 126 |
AK Chambon La Forêt | 079 |
AK Wingst | 056 |
Estimated Ap | 059 |
Estimated international sunspot number | 080 - Based on 17 stations |
Day | Begin | Max | Fine | Loc | Strength | OP | 10cm | Radio burst types | Catania/NOAA | |
---|---|---|---|---|---|---|---|---|---|---|
Nessuna |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
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