Issued: 2013 Jun 28 1234 UTC
Eruptive (C-class flares expected, probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
28 Jun 2013 | 098 | 026 |
29 Jun 2013 | 098 | 019 |
30 Jun 2013 | 098 | 007 |
Solar activity has been eruptive during the past 24 hours, featuring three C flares, from NOAA AR 11777 and 11778. The brightest flare was a C7.3 flare released by NOAA AR 11778 with peak time at 03:37 UT on June 28. More C flares are possible within the next 48 hours, with a chance for an M flare. NOAA AR 11777 released two CMEs (observed by LASCO C2 at 20:37 on June 27 and 02:00 on June 28). The first CME is not expected to be geo- effective, while there is a slight chance for a glancing blow from the second CME on July 1st. ACE detected a shock in the solar wind at 13:53 UT on June 27, probably due to some unidentified CME. The solar wind speed jumped from about 380 km/s to around 460 km/s, and has currently decreased again to 365 km/s. The IMF jumped from 3 to 8 nT, has subsequently further risen to 12 nT near 2h UT on June 28, and has since been gradually decreasing, with current values around 9 nT. Geomagnetic activity was at quiet to active levels (K Dourbes between 1 and 4) during the past 24 hours. Quiet to active conditions (K Dourbes < 4) are expected for June 28, with a chance for a minor geomagnetic storm (K Dourbes = 5). On June 29, quiet to active levels (K Dourbes = 4) with minor storm periods are possible as a consequence of the expected arrival at Earth of a new coronal hole high speed stream. Quiet geomagnetic levels (K Dourbes < 4) are likely on June 30.
Today's estimated international sunspot number (ISN): 050, based on 07 stations.
Wolf number Catania | 058 |
10cm solar flux | 100 |
AK Chambon La Forêt | 019 |
AK Wingst | 010 |
Estimated Ap | 009 |
Estimated international sunspot number | 043 - 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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The OVATION model predicts the Hemispheric Power Index to reach 50GW at 04:56 UTC
Active geomagnetic conditions (Kp4) Threshold Reached: 01:32 UTC
Moderate M2.5 flare
Minor R1 radio blackout in progress (≥M1 - current: M1.45)
Last X-flare | 2025/03/28 | X1.1 |
Last M-flare | 2025/04/01 | M2.5 |
Last geomagnetic storm | 2025/03/27 | Kp5 (G1) |
Spotless days | |
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Last spotless day | 2022/06/08 |
Monthly mean Sunspot Number | |
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February 2025 | 154.6 +17.6 |
April 2025 | 152.5 -2.1 |
Last 30 days | 130.7 -17.9 |