Issued: 2019 Oct 24 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Minor storm expected (A>=30 or K=5)
Quiet
10cm flux | Ap | |
---|---|---|
24 Oct 2019 | 065 | 036 |
25 Oct 2019 | 065 | 040 |
26 Oct 2019 | 065 | 022 |
Solar X ray flux remained below B level throughout the period. There are no active regions on disk and X-ray flux is expected to remain at background levels.
No Earth-directed CME's were detected in coronagraph images.
Solar high energy proton fluxes were at background levels and are expected to remain so.
Solar wind parameters showed this morning the expected arrival of the compression region ahead of the recurrent high speed stream. Total magnetic field reached a peak over 13nT around 9UT. The Bz was mostly negative with peaks down to -11nT. The magnetic field phi angle remained in the negative sector before switching to the positive sector around 11UT. The Solar wind speed increased to over 520km/s and is still rising. The Solar wind speed is expected to further increase and remain elevated for the next 24-48 hours before starting to subside.
Until just recently, geomagnetic conditions were quiet (NOAA Kp and local K Dourbes 0-2). The latest synoptic period 9-12UT showed active geomagnetic levels (NOAA Kp and local K Dourbes 4) as expected under the Solar wind perturbations. Geomagnetic conditions are expected to be active with minor geomagnetic storms and possibly a moderate geomagnetic storm period over the next 24-48 hours, before easing to unsettled to active levels.
Today's estimated international sunspot number (ISN): 000, based on 16 stations.
Wolf number Catania | 000 |
10cm solar flux | 065 |
AK Chambon La Forêt | /// |
AK Wingst | /// |
Estimated Ap | 003 |
Estimated international sunspot number | 000 - Based on 23 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 moderate possibility for aurora to appear at the following middle latitude regions in the near future
Surgut, SyktyvkarCurrent data suggests there is a slight possibility for aurora to appear at the following middle latitude regions in the near future
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Moderate G2 geomagnetic storm (Kp6) Threshold Reached: 16:34 UTC
Minor G1 geomagnetic storm (Kp5) Threshold Reached: 15:20 UTC
Strong G3 geomagnetic storm (Kp7) Threshold Reached: 14:18 UTC
Moderate G2 geomagnetic storm (Kp6) Threshold Reached: 13:21 UTC
The OVATION model predicts the Hemispheric Power Index to reach 125GW at 14:01 UTC
Last X-flare | 2025/03/28 | X1.1 |
Last M-flare | 2025/04/15 | M1.2 |
Last geomagnetic storm | 2025/04/15 | Kp6+ (G2) |
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 | 124.1 -10.1 |
Last 30 days | 124.7 -16.6 |