Issued: 2019 Jul 27 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
27 Jul 2019 | 068 | 005 |
28 Jul 2019 | 068 | 007 |
29 Jul 2019 | 068 | 007 |
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 are at nominal levels indicative of slow solar wind regime (300-3500 km/s). The total interplanetary magnetic field remained below 5 nT, the Bz component varied between -5 nT and +5 nT. The solar wind parameters might show some minor enhancements due to very mild effect of isolated small patchy polar coronal hole wind streams.
Quiet geomagnetic conditions were observed over the past 24 hours. Some short isolated unsettled conditions are possible due to the small coronal hole wind streams.
Today's estimated international sunspot number (ISN): 000, based on 16 stations.
Wolf number Catania | /// |
10cm solar flux | 068 |
AK Chambon La Forêt | 006 |
AK Wingst | 002 |
Estimated Ap | 002 |
Estimated international sunspot number | 000 - Based on 33 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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