Issued: 2018 May 05 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Minor storm expected (A>=30 or K=5)
Quiet
10cm flux | Ap | |
---|---|---|
05 May 2018 | 068 | 015 |
06 May 2018 | 069 | 052 |
07 May 2018 | 069 | 040 |
Solar activity was very low with X ray flux remaining below B level. Catania sunspot group 79 was shortlived while Catania sunspot group 80 was numbered NOAA 2708 (Beta; McIntosh Cro). Another region is rotating on the disk in the Northern hemisphere. The chance for any C class flares remains very low.
No Earth directed CMEs have been detected in coronagraph data.
The solar proton flux levels are at background values and are expected to remain so.
A shock was observed in the solar wind at 9:27UT with solar wind speed jumping from 340 to 370 km/s and total magnetic field from under 4nT to close to 7nT. Afterwards a further increase to a peak of near 12.5nT was observed. Bz became more volatile with a peak down to -9.5 nT. The shock is probably related to the upcoming interaction region and high speed stream from a negative polarity coronal hole although the magnetic field phi angle currently still indicates connection to a positive sector. Magnetic field is expected to remain elevated and perturbed and probably rising further. This will be followed by a further increase of the solar wind speed as the high speed stream sets in.
Geomagnetic conditions were quiet (local K Dourbes 1-2 and NOAA Kp 0-1). Geomagnetic conditions are likely to increase to active and minor geomagnetic storm levels with the passage of a sector boundary crossing and co-rotating interaction region in the next 24 hours. They will remain elevated as the high speed stream continues.
Today's estimated international sunspot number (ISN): 014, based on 21 stations.
Wolf number Catania | 023 |
10cm solar flux | 068 |
AK Chambon La Forêt | 007 |
AK Wingst | 006 |
Estimated Ap | 004 |
Estimated international sunspot number | 012 - Based on 23 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
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