Issued: 2019 Aug 20 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
20 Aug 2019 | 068 | 009 |
21 Aug 2019 | 067 | 011 |
22 Aug 2019 | 067 | 010 |
The solar activity has been quiet over the past 24 hours. The sun is currently spotless and the X-ray flux remained below B-level. Solar activity is expected to remain at low levels for the next 24 hours.
No Earth-directed coronal mass ejections (CME) were observed over the last 24 hours in the available coronagraph imagery. The greater than 10 MeV proton flux remained at background levels over the past 24 hours and is expected to remain at low levels.
The solar wind parameters show some enhancements starting from August 20, around 01:00 UT: The wind speed increased from 315 km/s to 425 km/s, the total interplanetary magnetic field reached 10 nT, and the Bz component varied between -7 nT and +7 nT (as recorded by ACE). The solar wind parameters may remain slightly enhanced for the next period due to the effect of a southern coronal hole of negative polarity that was facing Earth on August 18 in about two days.
Mostly quiet geomagnetic conditions were observed, Dourbes observed unsettled conditions (K=3) that can be associated with the effect of the southern coronal hole. Quiet to unsettled conditions are expected for the next period, with small chances of short periods of active conditions.
Today's estimated international sunspot number (ISN): 000, based on 20 stations.
Wolf number Catania | /// |
10cm solar flux | 068 |
AK Chambon La Forêt | 007 |
AK Wingst | 004 |
Estimated Ap | 004 |
Estimated international sunspot number | 000 - Based on 31 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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