INFO FROM SIDC - RWC BELGIUM 2019 May 26 12:30UTC

Over the past 24 hours solar activity has been very low. The visible solar
disc was spotless and no significant flares have been recorded. No Earth
directed Coronal Mass Ejections (CMEs) have been detected in the available
coronagraph imagery. The greater than 10MeV proton flux remained at
background levels over the past 24 hours. Solar activity is expected to
remain very low over the next 24 hours.

The solar wind was at background levels over the last 24 hours, gradually
increasing over the period from 300 km/s to 340 km/s. The total magnetic
field strength fluctuated between 0.2 and 4.9 nT. The Bz component ranged
between approximately -4 and +3.5 nT. 

Geomagnetic conditions have been quiet to unsettled over the past 24 hours,
with Kp index (NOAA) ranging between 0-2 and local K index (Dourbes)
ranging between 0-2, with one short interval of K equal to 3 at 18 UT on 25
May. Quiet geomagnetic conditions are expected over the next 24 hours.
Active intervals (K Dourbes = 4) are possible on May 28, due to the
expected arrival of a high speed solar wind stream associated with a
recurring, negative polarity equatorial coronal hole which began to
traverse the central meridian on 24 May.