Issued: 2018 Jun 15 1239 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
15 Jun 2018 | 072 | 006 |
16 Jun 2018 | 072 | 007 |
17 Jun 2018 | 072 | 007 |
Solar activity was very quiet with X-ray flux remaining below B level. Catania sunspot group 86 (NOAA active region 2713) is the only spotted region on the visible disk and it appears stable. Chances for C class flaring remain very low.
Only a small westbound CME was visible in SoHO/LASCO coronagraph images around 17:36UT which will not affect Earth.
Solar proton flux levels were at background values and are expected to remain so.
Solar wind conditions have been nominal with solar wind speed between 300-350 km/s and total magnetic field below 5 nT. The Bz component of the magnetic field was variable. The magnetic field phi angle indicates a negative sector connection. Solar wind conditions are expected to be nominal until at least June 18.
Geomagnetic conditions were quiet (local K Dourbes 1-2 and NOAA Kp 1) and are expected to remain so.
Today's estimated international sunspot number (ISN): 015, based on 18 stations.
Wolf number Catania | 017 |
10cm solar flux | 072 |
AK Chambon La Forêt | 008 |
AK Wingst | /// |
Estimated Ap | 007 |
Estimated international sunspot number | 016 - Based on 21 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
Current data suggests there is a slight possibility for aurora to appear at the following high latitude regions in the near future
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Last X-flare | 2025/03/28 | X1.1 |
Last M-flare | 2025/04/14 | M1.4 |
Last geomagnetic storm | 2025/04/06 | Kp5 (G1) |
Spotless days | |
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Last spotless day | 2022/06/08 |
Monthly mean Sunspot Number | |
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March 2025 | 134.2 -20.4 |
April 2025 | 132.1 -2.1 |
Last 30 days | 132.4 -10.7 |