INFO FROM SIDC - RWC BELGIUM 2020 Mar 29 12:30UTC

Solar flaring activity was at very low levels. No significant flares have
been recorded. Solar activity is expected to remain at very low levels. 

No Earth directed Coronal Mass Ejections (CMEs) were observed in the
available coronagraphic imagery. 

The greater than 10 MeV proton flux was at nominal levels over the past 24
hours and is expected to stay at nominal levels for the next 24 hours. The
greater than 2MeV electron flux was between nominal and moderate levels
over the past 24 hours and is expected to remain so for the next 24 hours.

The solar wind speed near Earth showed a generally increasing trend with
values ranging between 360 and 450 km/s (DSCOVR) over the past 24 hours.
The Interplanetary Magnetic Field (IMF) was predominantly oriented towards
the Sun (phi angle in the negative sector) with the magnitude varying
between 0 and 6 nT. Bz ranged between -5 and +5 nT. The solar wind
associated with an extension to the southern polar coronal hole, which
began to cross the central meridian on Mar 26, is expected to affect Earth
from late on Mar 29 until Mar 31.

Quiet to unsettled geomagnetic conditions were registered for the past 24
hours (K Dourbes and NOAA Kp recorded values 0-3 and 0-2, respectively).
Unsettled geomagnetic conditions are expected for the next 24 hours, with
active conditions (K Dourbes = 4) possible on Mar 30 and 31.