Issued: 2016 Oct 18 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
18 Oct 2016 | 078 | 013 |
19 Oct 2016 | 079 | 012 |
20 Oct 2016 | 080 | 017 |
Over the past 24 hours solar activity has been low. there were no significant flares and all Active Regions (AR) have shown low levels of activity. Solar protons have remained at background levels over the past 24 hours. Solar activity is expected to remain low over the next 24 hours with a low probability of C-class flares. There is evidence in EUV imagery (EUV wave and dimming) of a small eruption at 21:10 UT on 2016-Oct-17, from AR 2602 (Mcintosh class:Cao; Mag. type:Beta). As the source is near disk centre it may produce a halo CME in coronagraph imagery. However, Coronagraph imagery for this period is currently unavailable. The size of the wave and the dimming indicate a small eruption, but possibly Earth directed, if significant a PRESTO will be issued. The solar wind speed has been slowly decreasing from around between 750 and 600 km/s over the past 24 hours. The total magnetic field strength has remained around 5 nT. The Bz component fluctuated around 0 nT, ranging between -5 and +5 nT. Geomagnetic conditions ranged between Kp index 2-4 (NOAA) and local K index 2-4 (Dourbes) over the past 24 hours. The enhanced solar wind speeds are associated with a High Speed Stream (HSS) from a large negative polarity Southern polar coronal hole located in the western hemisphere. As the hole rotates towards the limb the speed is expected to abate. Geomagnetic conditions are expected to be quiet to unsettled.
Today's estimated international sunspot number (ISN): 029, based on 13 stations.
Wolf number Catania | 024 |
10cm solar flux | 076 |
AK Chambon La Forêt | 035 |
AK Wingst | 025 |
Estimated Ap | 025 |
Estimated international sunspot number | 029 - Based on 22 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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A southern hemisphere coronal hole is facing Earth. Enhanced solar wind could arrive in ~3 days
Active geomagnetic conditions (Kp4) Threshold Reached: 20:39 UTC
The OVATION model predicts the Hemispheric Power Index to reach 51GW at 18:18 UTC
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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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