INFO FROM SIDC - RWC BELGIUM 2017 Jun 23 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. AR 2664  (Mcintosh class:Hsx; Mag. type:Alpha) has produced
little activity. There’s a small centrally located filament channel which
looks stable, and a small northern coronal hole extending to lower
latitudes that has moved into the Western hemisphere and may increase solar
wind speeds in a couple of days. Solar activity is expected to remain low
over the next 24 hours with a low probability of C-class flares and a very
low probability of M-class flares.

The solar wind speed has fluctuated around 320 km/s over the past 24 hours.
The total magnetic field strength has fluctuated between 3 and 8 nT. The Bz
component fluctuated around 0 nT, but has been mainly positive. Geomagnetic
conditions ranged between Kp index 1-3 (NOAA) and local K index 0-3
(Dourbes) over the past 24 hours. Geomagnetic conditions are expected to be
quiet.