INFO FROM SIDC - RWC BELGIUM 2019 Nov 12 12:30UTC

The solar activity has been at very low levels over the past 24 hours. The
Sun is currently spotless and the X-ray flux remained below B-level. Solar
activity is expected to remain at low levels for the next 24 hours.

No earth-directed coronal mass ejections (CMEs) have been observed in the
available coronagraphic imagery.
The greater than 10 MeV proton flux was at nominal values. 

The solar wind was slightly enhanced over the past 24 hours: The total
magnetic field fluctuated around 10 nT, the solar wind speed varied around
315 km/s, and the southern component of the magnetic filed remained
positive. After this relatively short and minor disturbance, the solar wind
parameters are expected to return to the nominal level within the next 24
hours.

Quiet geomagnetic conditions were observed over the past 24 hours, and is
expected to remain so for the next period.