INFO FROM SIDC - RWC BELGIUM 2017 May 25 13:40UTC

Over the past 24 hours solar activity has been low. No significant flares
have been recorded. NOAA Active Region (AR) 2660 has been most active,
producing two B-class flares. No Earth directed Coronal Mass Ejections
(CMEs) have been detected in coronagraph observations. The greater than
10MeV proton flux remained at background levels over the past 24 hours.
Solar activity is expected to remain low over the next 24 hours with a
small chance for C-class flares.
Solar wind speed decreased from about 475 km/s to values around 370 km/s.
The total interplanetary magnetic field (IMF) strength, as recorded by the
DSCOVR satellite, was around 3.5 nT. Bz fluctuated between -2 and +3 nT.
Geomagnetic conditions (K Dourbes between 0 and 3; NOAA Kp between 0 and 1)
were ranged from quiet to unsettled level in the past 24 hours. Solar wind
speed is expected to decrease even more today. In response geomagnetic
conditions are likely to experience mostly quiet to unsettled conditions
today (25-May-2017 April) and tomorrow (26-May-2017). Active conditions
with a small chance for minor geomagnetic storm are possible on the day
three (27-May-2017) due to possible arrival of 23-May 2017 coronal mass
ejection.