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 2017 Jun 22 12:30UTC

Over the past 24 hours solar activity has been low. No significant flares
have been recorded. No Earth directed Coronal Mass Ejections (CMEs) have
been detected. AR 2664  (Mcintosh class:Hsx; Mag. type:Alpha) appears
complex in HMI magnetogram observations and has shown some evidence of
activity, producing several small narrow CMEs which may enhance activity
levels in the coming days. There's a small centrally located filament
channel which looks stable, and a small northern coronal hole located at
high latitudes and central longitudes, which is unlikely to significantly
affect the Earth system but may enhance solar wind speeds in several days.
Solar activity is expected to remain low over the next 24 hours with a low
probability of C-class flares and a very low probability of M-class flares.
The solar wind speed has fluctuated around 350 km/s over the past 24 hours.
The total magnetic field strength has fluctuated between 5 and 8 nT. The Bz
component fluctuated around -5 nT. Geomagnetic conditions ranged between Kp
index 1-3 (NOAA) and local K index 1-3 (Dourbes) over the past 24 hours.
Geomagnetic conditions are expected to be quiet.

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

2017 Jun 19 1130 UTC
In response to the recently issued PRESTO (issued on 2017-Jun-19 at 10:50 [more]

2017 Jun 17 1201 UTC
END OF ALL QUIET ALERT ...................... The SIDC [more]

2017 Apr 03 1504 UTC
A class M5.8 solar X-ray flare occurred on 2017/04/03 with peak time 14:29UT [more]

2016 Nov 05 1349 UTC
A halo or partial-halo CME was detected with the following characteristics: [more]


Science Highlights

Jun 21, 2017: A day on the Sun

Apr 26, 2017: Works in progress!...

Apr 20, 2017: Impressive solar eruption

Apr 11, 2017: Airplane transits the Sun!

Apr 05, 2017: M-class flares à volonté!

click here for all science highlights

Press

Jun 02, 2017: Extreme Ultraviolet Imager (EUI) ready for launch!

May 28, 2017: A coronal mass ejection as the source of a strong geomagnetic storm (NL-FR-EN)

Oct 26, 2016: High-speed solar wind causes major geomagnetic storm (NL-FR-EN)

Click here for all the press releases



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