Issued: 2016 May 01 1230 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
01 May 2016 | 094 | 014 |
02 May 2016 | 096 | 010 |
03 May 2016 | 098 | 007 |
Solar activity has been low, only one C-class flare in past 24 h: a C2.4 flare that peaked at 09:22 UT from NOAA AR 2539 (Catania 66 and 67). Six active regions are visible on the disk, three of them with beta magnetic field configuration and the rest with alpha magnetic field configuration of their photospheric field. C-class flaring is likely for the next 24 h.
Geomagnetic conditions have been quiet. Solar wind speed is at 375 km/s with interplanetary magnetic field magnitude of 10 nT. Active conditions (with isolated minor storm periods) are expected when the fast speed stream from a coronal hole arrives to the Earth later today.
Today's estimated international sunspot number (ISN): 085, based on 13 stations.
Wolf number Catania | /// |
10cm solar flux | 094 |
AK Chambon La Forêt | 014 |
AK Wingst | 008 |
Estimated Ap | 008 |
Estimated international sunspot number | /// - Based on /// 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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