INFO FROM SIDC - RWC BELGIUM 2019 May 20 12:30UTC

Over the past 24 hours solar activity has been low. No significant flares
have been recorded. No Earth directed Coronal Mass Ejections (CMEs) have
been detected.  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.

The solar wind speed has fluctuated between 350 and 415 km/s over the past
24 hours. The total magnetic field strength fluctuated around 6 nT for the
first part of the period and then slowly increased to a maximum of around 9
nT at around 7:00 UT. The Bz component fluctuated around 0 nT, ranging
between -6.3 and +7.7 nT.

Geomagnetic conditions ranged between Kp index 0-3 (NOAA) and local K index
0-3 (Dourbes) over the past 24 hours. Quiet to unsettled geomagnetic levels
are expected to continue. Some isolated active intervals are also possible,
due to the expected arrival of a weak solar wind stream associated with a
recurring, negative polarity equatorial coronal hole which traversed the
central meridian on 18 May.