Issued: 2016 Apr 03 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
03 Apr 2016 | 080 | 014 |
04 Apr 2016 | 081 | 018 |
05 Apr 2016 | 082 | 018 |
Solar flaring activity was restricted to a single B2 event at the start of the period. NOAA 2526 remained quiet. No earth-directed coronal mass ejections (CMEs) were observed. The x-ray background flux was steady at the A7 level.
Quiet conditions are expected to continue.
The Kp index reached minor storming levels on 2 April during the 15-18UT interval, and moderate geomagnetic storming during the 21-24UT interval. K Dourbes was resp. at minor storming and active conditions. This geomagnetic activity was the result of the arrival of a co-rotating interaction region and associated wind stream from a negative coronal hole.
Solar wind speeds continued to gradually increase from about 330 km/s at 08:00UT to about 530 km/s around 21:30UT. A sharp drop in wind density from 40 to 7 particles per cm3 occurred at 14:05UT, coinciding with a final shift in the direction of the interplanetary magnetic field from away to towards the Sun. It was followed about an hour later by a strong dive of Bz towards negative values around -14 nT, with sustained but gradually weakening negative values over the subsequent 7 hours.
Currently, wind speed is declining with values near 400 km/s, and Bz varying between -5 and +5 nT. Mostly unsettled to active geomagnetic conditions are expected for the rest of the day (3 April), a minor storming episode not excluded. The wind stream from an elongated negative coronal hole between latitudes +10 and +30 degrees is still expected to influence the earth environment starting from 4 April onwards.
Today's estimated international sunspot number (ISN): 013, based on 18 stations.
Wolf number Catania | /// |
10cm solar flux | 082 |
AK Chambon La Forêt | 041 |
AK Wingst | 023 |
Estimated Ap | 019 |
Estimated international sunspot number | 012 - Based on 20 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
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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 |
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