Welcome to the Solar Influences Data Analysis Center (SIDC), which is the solar physics research department of the Royal Observatory of Belgium. The SIDC includes the World Data Center for the sunspot index and the ISES Regional Warning Center Brussels for space weather forecasting.

INFO FROM SIDC - RWC BELGIUM 2014 Nov 26 12:25:23

Four C-class flare were observed, with NOAA 2217 producing the strongest
event of the period (C2.9 peaking at 06:17UT). Slowly developing region
NOAA 2219 and a new, currently unnumbered, region near the east limb merit
some attention, as they were the sources of the other C-class flares.
Numerous, but quiet, filaments are present on the solar disk, with the
longest measuring 40 degrees and located in the NE quadrant. No
Earth-directed CMEs were observed.

Further C-class flaring is expected, with a small chance on an isolated
M-class flare.

Solar wind speed declined from about 400 to 320 km/s. Bz was mostly
negative and varied between -6 and +4 nT. The IMF is directed away from the
Sun. The geomagnetic field was quiet to unsettled (K<4), and is expected to
remain so. Effects from an expected Sector Boundary Crossing and the
possible high speed stream from the extension of a coronal hole may result
in an isolated active period on 27-28 November.

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

Most recent alerts

2014 Nov 12 1241 UTC
The partial halo CME, first seen in the SOHO LASCO C2 field of view at [more]

2014 Nov 08 0749 UTC
A halo or partial-halo CME was detected with the following characteristics: [more]

2014 Aug 08 1211 UTC
END OF ALL QUIET ALERT ...................... The SIDC [more]

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Nov 07, 2014: NOAA 2205 produces an X1.6 flare (NL-FR-EN) - UPDATED

Nov 05, 2014: The "All Saints" filament eruption

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