INFO FROM SIDC - RWC BELGIUM 2020 Mar 25 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 in the past 24
hours and is expected to stay at nominal levels in the next 24 hours. The
greater than 2 MeV electron flux is enhanced (briefly crossing the event
threshold of 1000 pfu between 14:30 and 19:30 Mar 24). It is expected to
remain enhanced on Mar 25 and then to slowly return to nominal values.

The solar wind speed near Earth showed a generally decreasing trend with
values ranging between 370 and 460 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) and its magnitude varied between
2 and 6 nT. Bz ranged between -4 and +5 nT. Background solar wind
conditions are expected for the next 24 hours.

Quiet geomagnetic conditions were registered for the past 24 hours (K
Dourbes and NOAA Kp recorded values of between 0 and 2). Mostly quiet
geomagnetic conditions are expected on March 25 to 27.