Issued: 2018 Jul 31 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
31 Jul 2018 | 068 | 005 |
01 Aug 2018 | 068 | 008 |
02 Aug 2018 | 068 | 006 |
Solar activity was at very low levels. A small filament located at N15E20 slowly erupted on 31 July between 04 and 07UT. No x-ray flaring or obvious coronal dimming was associated with the event. No coronal mass ejections (CMEs) were observed in available coronagraphic imagery. The greater than 10 MeV proton flux was at nominal levels.
Solar activity is expected to remain at very low levels.
Solar wind speed varied between 300 and 340 km/s (DSCOVR). Bz was mostly negative during the first half of the period, and positive during the second half, varying between -6 and +5 nT. The interplanetary magnetic field turned to a predominately away direction (positive sector) around 01UT. Mostly quiet geomagnetic conditions were observed, with some unsettled intervals recorded by Dourbes.
Mostly quiet to unsettled geomagnetic conditions are expected.
Today's estimated international sunspot number (ISN): 000, based on 20 stations.
Wolf number Catania | /// |
10cm solar flux | 068 |
AK Chambon La Forêt | /// |
AK Wingst | 007 |
Estimated Ap | 005 |
Estimated international sunspot number | 000 - Based on 37 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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