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

Solar activity was at very low levels. While rounding the west limb, NOAA
2738 produced 4 B-class flares, the strongest being a B8 flare peaking at
00:50UT. The lone sunspot group currently visible on the solar disk, NOAA
2739, was quiet and is decaying. No earth-directed coronal mass ejections
were observed over the last 24 hours. The greater than 10 MeV proton flux
was at nominal values. An equatorial negative polarity coronal hole (CH) is
transiting the central meridian.

Solar activity is expected to remain at very low levels.

Solar wind speed was fairly steady between 300 and 350 km/s (DSCOVR). Bz
varied between -4 and +6 nT. The interplanetary magnetic field was mostly
directed away from the Sun (positive sector) until about 07:00UT, when it
switched back to towards the Sun (negative sector). Geomagnetic conditions
were at quiet levels, with an isolated unsettled interval (14-17UT)
recorded at Dourbes. 

Quiet geomagnetic conditions are expected to continue, with a chance on an
unsettled interval.