Issued: 2018 Aug 16 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
16 Aug 2018 | 069 | 013 |
17 Aug 2018 | 069 | 012 |
18 Aug 2018 | 069 | 007 |
The solar activity has been quiet over the past 24 hours. The sunspot group (NOAA 2718) remained stable 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 solar protons flux remained at nominal levels over the past 24 hours and is expected to remain so.
Over the past 24 hours, the solar wind measurements continued to be enhanced with the solar wind associated to the Coronal Hole (which has crossed the central meridian on August 11). The wind speed increased from 450 km/s to about 500 km/s; The interplanetary magnetic field strength fluctuated between 3 and 13 nT; The Southward magnetic component fluctuated between -8 and 10 nT. The enhanced solar wind conditions are expected to persist for the next 24 hours and start to decline on August 18.
Due to the enhanced solar wind conditions, the geomagnetic conditions was unsettled to active (K-Dourbes and Kp were ranging between 2 and 4). Unsettled conditions is expected until while the Earth remains under the influence of the solar wind associated to the coronal hole. Active conditions are likely especially if the southward magnetic component remains negative for longue periods.
Today's estimated international sunspot number (ISN): 013, based on 18 stations.
Wolf number Catania | /// |
10cm solar flux | 069 |
AK Chambon La Forêt | 030 |
AK Wingst | 020 |
Estimated Ap | 020 |
Estimated international sunspot number | 013 - Based on 19 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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