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 2019 Jun 19 12:30UTC

Solar activity was at very low levels. The Sun remains spotless and no
significant flares have been recorded.  No Earth directed coronal mass
ejections (CMEs) were observed over the last 24 hours in the available
coronagraph imagery. The greater than 10 MeV proton flux was at nominal
values. Solar activity is expected to remain at very low levels. 

The solar wind fluctuated between 300 and 340 km/s (DSCOVR). Bz varied
between -4 and +4 nT. The interplanetary magnetic field was predominantly
directed away from the Sun (positive sector), but switched to be directed
towards the Sun from approximately 8 UT on June 19. Quiet to unsettled
geomagnetic conditions were observed, with the Kp index (NOAA) registering
1 and the local K index (Dourbes) ranging between 1-3 over the past 24
hours.

Quiet geomagnetic conditions are expected, with some unsettled periods due
to the solar wind streams associated with a series of fragmented negative
polarity coronal holes. The possibility of isolated active periods is also
not excluded.

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

2019 Jun 09 1213 UTC
A small filament eruption was seen at approximately 00:00 UT yesterday [more]

2019 Jun 09 1206 UTC
END OF ALL QUIET ALERT ...................... The SIDC [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]