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 2018 Dec 16 12:30UTC

NOAA 2731 produced a B1.0 flare in the past 24 hours, and has decayed to an
alpha region. The chance for a C flare in the next 24 hours is estimated at
5%.

No Earth-directed Coronal Mass Ejections (CMEs) were observed in 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 in the next 24 hours.

Solar wind speed near Earth as registered by DSCOVR varied between about
300 and 350 km/s in the past 24 hours. The Interplanetary Magnetic Field
(IMF) was predominantly directed towards the Sun and its magnitude varied
between about 0 and 4 nT. Bz was never below -5 nT. A weak solar wind
stream associated with a negative polarity, equatorial-South polar coronal
hole may arrive near Earth on December 16.

Quiet geomagnetic conditions (K Dourbes between 0 and 1; NOAA Kp between 0
and 1) were registered in the past 24 hours. There is a chance for active
intervals (K Dourbes = 4) on December 16 and 17, related to the possible 
arrival of a weak solar wind stream associated with a negative polarity,
equatorial-South polar coronal hole. Quiet to unsettled geomagnetic levels
(K Dourbes < 4) are expected on December 18.

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

2018 Dec 14 1120 UTC
END OF ALL QUIET ALERT ...................... The SIDC [more]

2018 Nov 05 1320 UTC
Geomagnetic conditions have reached moderate storm levels on a planetary [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]