Issued: 2016 Apr 08 1246 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
08 Apr 2016 | 093 | 004 |
09 Apr 2016 | 091 | 007 |
10 Apr 2016 | 090 | 008 |
Over the past 24 hours solar activity has been low. The largest flare was a B7.7 class flare, produced by Active Region (AR) 2529 (Macintosh class:Hkx; Mag. Type:Alpha), which peaked yesterday at 13:37 UT. This AR 2528 is currently the only significant region on disk with evidence of small amounts of flux cancellation in HMI magnetogram observations. Another AR 2528 (Macintosh class:Cao; Mag. Type:Beta), is moving onto the West limb. A Coronal Mass Ejection(CME) detected yesterday at 08:36 UT originated at the West Limb has some probability to hit the Earth in approximately 3 days time. The initial median speed of CME is 450 km/s, which is higher than the background median solar wind speed 400 km/s. 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. The solar wind parameters have been affected by the sector boundary crossing from 17:30 UT 07-Apr-16 till 04:00 UT today. The total magnetic field strength in solar wind has increased till 14 nT, while Bz component of the magnetic field decreased till -14 nT simultaneously with the transition of the Phi angle. The solar wind speed however remained stable varying around 400 km/s over the past 24 hours. As the consequence a minor magnetic storm has occurred detected at 24:00 UT today, which lasted approximately till 08:00 UT today. Geomagnetic indexes as detected this morning (Kp index = 5 (NOAA), local K index = 6 (Dourbes) at and Dst Kioto = 72 nT) are returning to the quiet unperturbed conditions now ( Kp = 1, K = 2, Dst = 45 nT). Quiet conditions are expected next 2 days. However enhanced solar wind conditions are again possible starting from 11-04-16 due to CME detected yesterday at the West limb of the Sun.
Today's estimated international sunspot number (ISN): 027, based on 11 stations.
Wolf number Catania | /// |
10cm solar flux | 092 |
AK Chambon La Forêt | 039 |
AK Wingst | 022 |
Estimated Ap | 020 |
Estimated international sunspot number | 018 - 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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Minor G1 geomagnetic storm (Kp5) Threshold Reached: 13:07 UTC
The OVATION model predicts the Hemispheric Power Index to reach 75GW at 13:21 UTC
Minor G1 geomagnetic storm (Kp5) Threshold Reached: 23:59 UTC
Minor G1 geomagnetic storm (Kp5) Threshold Reached: 20:02 UTC
The OVATION model predicts the Hemispheric Power Index to reach 50GW at 13:56 UTC
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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March 2025 | 134.2 -20.4 |
April 2025 | 143 +8.8 |
Last 30 days | 130.4 -16.1 |