SIDC Ursigram

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PRESTO FROM SIDC - RWC BELGIUM Wed May 23 2012, 1231 UT

Catania sunspot group 39 (NOAA AR 1484) produced a C1.2 flare peaking at 00:27 UT today. More C-class flares can be expected from this group, as well as from recently emerged Catania sunspot group 47 (NOAA AR 1488).
The post-shock solar wind flow was followed by a fast solar wind stream (with the speed reaching 700 km/s) from a small low-latitude coronal hole in the southern hemisphere. Due to high interplanetary magnetic field (IMF) magnitude (that reached 15 nT), active geomagnetic conditions (K = 4) were reported by Dourbes and IZMIRAN and minor storm conditions (K = 5) were reported by NOAA. Currently the solar wind speed is still elevated (around 620 km/s), but the IMF magnitude decreased to average values (around 4 nT). We therefore expect quiet geomagnetic conditions.


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presto
2012 May 22 0903 UTC
After the arrival of the interplanetary shock yesterday evening, the interplanetary [more]

cactus
2012 May 17 2117 UTC
A halo or partial-halo CME was detected with the following characteristics: [more]

flaremail
2012 May 10 0456 UTC
A class M5.7 solar X-ray flare occurred on 2012/05/10 with peak time 04:18 [more]

quieta
2011 Jun 30 1308 UTC
END OF ALL QUIET ALERT ...................... The SIDC - RWC Belgium expects [more]




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