Issued: 2015 Jul 26 1230 UTC
C-class flares expected, (probability >=50%)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
26 Jul 2015 | 098 | 008 |
27 Jul 2015 | 103 | 008 |
28 Jul 2015 | 109 | 012 |
There are currently 2 sunspot groups visible on the solar disk. NOAA 2389 is small and produced only B-class flares. NOAA 2390 shows some mixed magnetic polarity mixing in its asymmetric trailing portion. No C-class flares were recorded. Two significant coronal mass ejections (CMEs) were observed on 25 July starting resp. at 14:48UT (northwest) and 19:24UT (northeast), but they were both backside events. No earth-directed CMEs were observed.
There's a reasonable chance on C-class flares.
Solar wind speed varied mostly between 390 and 450 km/s, while Bz fluctuated between -6 and +6 nT under the influence from a moderate-speed stream from the northern coronal hole (CH) starting around 18:00UT on 25 July. Mostly quiet to unsettled geomagnetic conditions were observed. The wind stream from a small equatorial positive coronal hole (CH) may influence the earth environment on 28-29 July.
Mostly quiet to unsettled geomagnetic conditions are expected, with a small chance on an active episode.
Today's estimated international sunspot number (ISN): 043, based on 15 stations.
Wolf number Catania | /// |
10cm solar flux | 094 |
AK Chambon La Forêt | 015 |
AK Wingst | 011 |
Estimated Ap | 010 |
Estimated international sunspot number | 036 - Based on 20 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
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