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
A lot of people come to SpaceWeatherLive to follow the Solar activity or if there is a chance to see the aurora, but with more traffic comes higher costs to keep the servers online. If you like SpaceWeatherLive and want to support the project you can choose a subscription for an ad-free site or consider a donation. With your help we can keep SpaceWeatherLive online!
| Last X-flare | 2025/12/08 | X1.1 |
| Last M-flare | 2025/12/09 | M1.5 |
| Last geomagnetic storm | 2025/12/04 | Kp5 (G1) |
| Spotless days | |
|---|---|
| Last spotless day | 2022/06/08 |
| Monthly mean Sunspot Number | |
|---|---|
| November 2025 | 91.8 -22.8 |
| December 2025 | 160.6 +68.8 |
| Last 30 days | 108 +10.6 |