The SIDC is part of the Royal Observatory of Belgium and a partner in the Solar Terrestrial Center of Excellence (STCE).

INFO FROM SIDC - RWC BELGIUM 2020 Mar 27 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 for the next 24 hours. The
greater than 2MeV electron flux was slightly enhanced on Mar 26. It has
since returned to nominal levels and is expected to remain at nominal
levels for the next 24 hours.

The solar wind speed near Earth fluctuated around 400 km/s (DSCOVR) over
the past 24 hours. The magnitude of the Interplanetary Magnetic Field (IMF)
varied between 1 and 6 nT and the phi angle was mostly negative with
several short deviations into the positive sector. Bz ranged between -5 and
+4 nT. Background solar wind conditions are expected for the next 24 hours.
The solar wind associated with an extension to the southern polar coronal
hole, which began to cross the central meridian on Mar 26, is expected to
affect Earth from March 29.

Quiet to unsettled geomagnetic conditions were registered for the past 24
hours (K Dourbes and NOAA Kp recorded values 1-3). Quiet to unsettled
geomagnetic conditions are expected for the next 24 hours, with active
conditions (K Dourbes = 4) possible from late on Mar 29.

Latest SWAP image

SWAP latest image

Latest USET H-alpha image
USET latest Halpha image

Latest LYRA curve

Latest LYRA Curves

Latest Callisto Observations

Latest HUMAIN Callisto qkl

Daily estimated sunspot number
EISN

Most recent alerts

2020 Feb 20 1308 UTC
START OF ALL QUIET ALERT ........................ The SIDC - RWC Belgium [more]

2019 Oct 25 0924 UTC
Geomagnetic conditions have reached moderate storm levels (NOAA Kp=6 for [more]

2018 May 04 1644 UTC
A halo or partial-halo CME was detected with the following characteristics: [more]

2017 Sep 10 1650 UTC
A class X8.9 solar X-ray flare occurred on 2017/09/10 with peak time 16:06UT [more]