Emesso: 2018 Dec 04 1233 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
04 Dec 2018 | 067 | 008 |
05 Dec 2018 | 068 | 006 |
06 Dec 2018 | 068 | 007 |
The solar activity has been quiet over the past 24 hours. The visible solar disc remained spotless, and no significant flare has been recorded. Quiet flaring conditions are expected for the next 24-hour period.
No Earth directed Coronal Mass Ejection has been observed. The greater than 10 MeV solar protons flux remained at nominal levels over the past 24 hours and is expected to remain so.
The solar wind measurements remained under the influence of the enhanced solar wind associated with the Coronal Hole (which reached the central meridian on November 27). The wind speed reached 506 km/s on December 3, around 13.00 UT and then slowly decreased to the current value of 406 km/s; The interplanetary magnetic field strength fluctuated between 4 and 9 nT and the southward magnetic component between -7 and 7 nT. The solar wind parameters are expected decrease and return towards an ambient background and slow solar wind speed regime. Moreover, a CME was observed headed south on December 30 with low speed. The northern flank of this CME may glance Earth later today or earlier on December 5. Slightly enchantment of the solar wind parameters might be observed.
The geomagnetic conditions were quiet to unsettled with a short period of active condition observed by the local station in Dourbes (K-Dourbs=4) on December 3, at 17:00 UT. The conditions are expected to be mainly quiet (short unsettled period cannot be excluded) as the Earth is entering the slow solar wind speed regime..
Today's estimated international sunspot number (ISN): 000, based on 20 stations.
Wolf number Catania | 000 |
10cm solar flux | 068 |
AK Chambon La Forêt | 018 |
AK Wingst | /// |
Estimated Ap | 011 |
Estimated international sunspot number | 000 - Based on 19 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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