Issued: 2013 Oct 14 1310 UTC
Active (M-class flares expected, probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
14 Oct 2013 | 130 | 010 |
15 Oct 2013 | 130 | 007 |
16 Oct 2013 | 130 | 011 |
Several C-class flares in past 24h, the strongest being a C4.5 flare peaking at 17:58 UT on October 13, from NOAA AR 1861 (beta gamma magnetic field configuration). This AR, and in particular AR 1865 (beta-gamma- delta), can produce M-class flares in the next 48h. Geomagnetic conditions are currently unsettled due to the arrival of a fast speed stream from a coronal hole. The solar wind speed is at 500 km/s with magnetic field intensities currently at 7 nT. Conditions may reach active levels.
Today's estimated international sunspot number (ISN): 097, based on 09 stations.
Wolf number Catania | /// |
10cm solar flux | 129 |
AK Chambon La Forêt | 006 |
AK Wingst | 002 |
Estimated Ap | 002 |
Estimated international sunspot number | 094 - Based on 15 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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Active geomagnetic conditions (Kp4) Threshold Reached: 22:47 UTC
The OVATION model predicts the Hemispheric Power Index to reach 50GW at 21:37 UTC
Active geomagnetic conditions (Kp4) Threshold Reached: 01:41 UTC
Last X-flare | 2025/03/28 | X1.1 |
Last M-flare | 2025/04/08 | M1.5 |
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 | 141.4 +7.2 |
Last 30 days | 137.9 +0.4 |