Emesso: 2019 Apr 16 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
16 Apr 2019 | 075 | 007 |
17 Apr 2019 | 074 | 006 |
18 Apr 2019 | 074 | 005 |
Solar activity was at very low levels. NOAA 2738 produced a B3 flare peaking at 19:31UT. No earth-directed coronal mass ejections were observed over the last 24 hours. The greater than 10 MeV proton flux was at nominal values. A weak extension from the positive polarity northern polar coronal hole (CH) is transiting the central meridian.
Solar activity is expected to remain at very low levels.
Solar wind speed continued its gradual increase from its initial 340 km/s to reach 400 km/s by the end of the period. Bz varied between -6 and 6 nT, with a negative stretch from 15 till 20UT. The interplanetary magnetic field was mostly directed towards the Sun (negative sector). Quiet to unsettled geomagnetic conditions were observed.
Quiet to unsettled geomagnetic conditions are expected to continue.
Today's estimated international sunspot number (ISN): 012, based on 23 stations.
Wolf number Catania | /// |
10cm solar flux | 075 |
AK Chambon La Forêt | 014 |
AK Wingst | /// |
Estimated Ap | 009 |
Estimated international sunspot number | 013 - Based on 33 stations |
Day | Begin | Max | Fine | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
---|---|---|---|---|---|---|---|---|---|---|
Nessuna |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
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