Issued: 2014 Jun 29 1251 UTC
Eruptive (C-class flares expected, probability >=50%)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
29 Jun 2014 | 115 | 007 |
30 Jun 2014 | 120 | 007 |
01 Jul 2014 | 125 | 007 |
The ARs rotating over the east limb into the visible disk are producing most of the activity at present. The strongest flare was a C4.9 with peak at 11:52 UT, originating in NOAA AR 2104 (no Catania number). This AR, and NOAA AR 2102 (no Catania number), will most likely produce more C-class and probably M-class flares. With solar wind speeds around 350 km/s and interplanetary magnetic field with a magnitude of 3 nT geomagnetic conditions are quiet and expected to remain so.
Today's estimated international sunspot number (ISN): 057, based on 11 stations.
Wolf number Catania | /// |
10cm solar flux | 115 |
AK Chambon La Forêt | 014 |
AK Wingst | 008 |
Estimated Ap | 008 |
Estimated international sunspot number | 044 - Based on 16 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
Last X-flare | 2025/03/28 | X1.1 |
Last M-flare | 2025/04/05 | M1.0 |
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 | 148.7 +14.5 |
Last 30 days | 134.1 -5.6 |