Issued: 2014 Jul 31 1233 UTC
Active (M-class flares expected, probability >=50%)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
31 Jul 2014 | 160 | 004 |
01 Aug 2014 | 166 | 004 |
02 Aug 2014 | 172 | 018 |
There are currently 8 sunspot groups present on the solar disk. NOAA 2127 produced most of the flares including a C9 flare peaking at 16:17UT (30 July). Overnight, NOAA 2130 developed a delta spot south of its trailing portion and started producing flares again around 05:00UT. This culminated in an M2.5 flare peaking at 11:14UT, the strongest event of the period. Evaluation of any associated CME is pending the availability of coronagraphic images. Yesterday's filament eruption (NE quadrant) was associated to a CME which may have an Earth directed component. Based on STEREO and SOHO imagery, its true speed is estimated to be about 800 km/s and may affect the geomagnetic field on 2 August. The filaments near the NE-limb and in the SW solar quadrant are stable. Further M-class flaring is possible, in particular from NOAA 2127 and 2130. Solar wind speed varied between 300 and 350 km/s, and Bz between -3 and +4 nT. Quiet geomagnetic conditions were observed. A small equatorial coronal hole is approaching the central meridian and may influence the geomagnetic field around 4 August. Quiet geomagnetic conditions are expected until 2 August, when the CME related to the 30 July filament eruption may deliver a glancing blow and result in active geomagnetic conditions.
Today's estimated international sunspot number (ISN): 101, based on 22 stations.
Wolf number Catania | /// |
10cm solar flux | 152 |
AK Chambon La Forêt | 006 |
AK Wingst | 004 |
Estimated Ap | 004 |
Estimated international sunspot number | 098 - Based on 28 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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