Emesso: 2013 Jun 30 1259 UTC
Eruptive (C-class flares expected, probability >=50%)
Minor storm expected (A>=30 or K=5)
Quiet
10cm flux | Ap | |
---|---|---|
30 Jun 2013 | 102 | 021 |
01 Jul 2013 | 105 | 030 |
02 Jul 2013 | 107 | 007 |
Solar activity has been eruptive during the past 24 hours, featuring two low C flares from NOAA 11778 and NOAA 11781. More C flares are possible within the next 48 hours, with a slight chance for an M flare, especially from NOAA AR 11778, 11780 and 11781. Solar wind density increased around 5:00 UT on June 29, while wind speed and temperature began to rise, marking the arrival of the expected coronal hole high speed stream. Meanwhile, solar wind speed has increased from about 360 km/s to 500 km/s. In the past 24 hours, geomagnetic activity has been at quiet to active levels (K Dourbes between 1 and 4; NOAA Kp between 2 and 4). A rise to minor storm levels is possible on June 30 and the first half of July 1st, due to an expected glancing blow from the CME of 02:00 UT on June 28. Quiet to active levels are likely in the second half of July 1st, and a return to quiet levels is expected on July 2nd.
Today's estimated international sunspot number (ISN): 050, based on 14 stations.
Wolf number Catania | /// |
10cm solar flux | 100 |
AK Chambon La Forêt | 037 |
AK Wingst | 035 |
Estimated Ap | 048 |
Estimated international sunspot number | 045 - Based on 22 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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