Välja antud: 2016 Oct 31 1349 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
31 Oct 2016 | 076 | 013 |
01 Nov 2016 | 077 | 008 |
02 Nov 2016 | 076 | 008 |
Solar activity is low. No flares were observed. There is one NOAA active region (AR 2604) on the visible side of the solar disc with the simple magnetic configuration (beta). Catania decaying (51) sunspot group is also observed on the visible side of solar disc. Cactus detected a slow- moving narrow CME yesterday 30-Oct-2016 at 23:36 UT at the western limb of the solar disk, with no geoeffective effects expected. One big, but stable filament is approaching solar disk centre. Solar proton flux intensity is expected to lie within the background levels. Solar activity is expected to be low with small probability for C-class flares.
Earth remained under the decaying influence of the high speed stream from the coronal hole. Solar wind speed decreased from around 600 km/s to 490 km/s (DSCOVR). The interplanetary magnetic field (Bt) decreased from about 10 nT to +4nT. Bz oscillated mostly between -4 and +4 nT. The local K index at Dourbes was ranged between 2 and 4(planetary Kp index was also ranged between 2 and 4) during last 24 hours. The geo-environment is expected to remain under the gradually weakening influence of the CH HSS. Quiet conditions are expected.
Today's estimated international sunspot number (ISN): 014, based on 28 stations.
Wolf number Catania | /// |
10cm solar flux | 076 |
AK Chambon La Forêt | 026 |
AK Wingst | 020 |
Estimated Ap | 022 |
Estimated international sunspot number | 014 - Based on 30 stations |
Day | Begin | Max | Lõpp | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
---|---|---|---|---|---|---|---|---|---|---|
Puuduvad |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
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