Issued: 2019 Mar 28 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
28 Mar 2019 | 069 | 010 |
29 Mar 2019 | 068 | 010 |
30 Mar 2019 | 067 | 008 |
There are no active regions, presently observed on the visible side of the solar disc, and accordingly solar flaring activity is very low. We expect such a low level of the solar activity, without C-class and even B-class flares, to persist in the coming hours. There were no wide and/or Earth directed CMEs reported and the solar protons remained at the background level.
At about 03:40 UT this morning, interplanetary magnetic field magnitude increased (to the value of about 14 nT) simultaneously with the increase of the solar wind speed and decrease of the temperature indicating arrival of possibly either ICME (still unclear what would be its solar counterpart) or a structure at the boundary between the slow and the fast solar wind. More will be reported later, when larger part of the structure becomes visible in the in situ observations. The solar wind speed is presently about 430 km/s and the interplanetary magnetic field magnitude is presently 9 nT. The fast solar wind associated with the negative polarity equatorial coronal hole which reached central meridian on March 25 is expected at the Earth tomorrow. The geomagnetic conditions are quiet to unsettled (both local station at Dourbes and NOAA reported only K=3 and Kp=3, respectively) and we expect them to stay so in the coming hours.
Today's estimated international sunspot number (ISN): 000, based on 14 stations.
Wolf number Catania | /// |
10cm solar flux | 069 |
AK Chambon La Forêt | 011 |
AK Wingst | 008 |
Estimated Ap | 008 |
Estimated international sunspot number | 000 - Based on 25 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 Sun's activity or if there is aurora to be seen, but with more traffic comes higher server costs. Consider a donation if you enjoy SpaceWeatherLive so we can keep the website online!
Last X-flare | 2025/03/28 | X1.1 |
Last M-flare | 2025/04/01 | M2.4 |
Last geomagnetic storm | 2025/03/27 | Kp5 (G1) |
Spotless days | |
---|---|
Last spotless day | 2022/06/08 |
Monthly mean Sunspot Number | |
---|---|
February 2025 | 154.6 +17.6 |
April 2025 | 147 -7.6 |
Last 30 days | 128.8 -21.8 |