INFO FROM SIDC - RWC BELGIUM 2017 Jun 22 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) appears
complex in HMI magnetogram observations and has shown some evidence of
activity, producing several small narrow CMEs which may enhance activity
levels in the coming days. There's a small centrally located filament
channel which looks stable, and a small northern coronal hole located at
high latitudes and central longitudes, which is unlikely to significantly
affect the Earth system but may enhance solar wind speeds in several 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 350 km/s over the past 24 hours.
The total magnetic field strength has fluctuated between 5 and 8 nT. The Bz
component fluctuated around -5 nT. Geomagnetic conditions ranged between Kp
index 1-3 (NOAA) and local K index 1-3 (Dourbes) over the past 24 hours.
Geomagnetic conditions are expected to be quiet.