Issued: 2015 Sep 03 1230 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
03 Sep 2015 | 088 | 017 |
04 Sep 2015 | 087 | 007 |
05 Sep 2015 | 086 | 007 |
Solar activity has been low in past 24 h, only one C-class flare occurred: C1.7 peaking at 11:37 UT from NOAA AR 2407, that rotated behind the west limb already. More C-class flares are possible. Solar wind speeds have been increasing steadily in past 24 h (from 350 to 450 km/s), marking the expected arrival of the fast speed stream from a coronal hole. A sector boundary crossing was detected also at 15:10 UT on September 2. The interplanetary magnetic field intensity is at 7 nT, only unsettled geomagnetic conditions have been recorded. Active to minor storm periods are possible in the coming 24 h considering the increase in solar wind speed continues.
Today's estimated international sunspot number (ISN): 028, based on 14 stations.
Wolf number Catania | 044 |
10cm solar flux | 088 |
AK Chambon La Forêt | 014 |
AK Wingst | 010 |
Estimated Ap | 009 |
Estimated international sunspot number | 038 - Based on 23 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
Current data suggests there is a slight possibility for aurora to appear at the following high latitude regions in the near future
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