:Issued: 2010 Apr 02 1342 UTC :Product: documentation at http://www.sidc.be/products/meu #--------------------------------------------------------------------# # DAILY BULLETIN ON SOLAR AND GEOMAGNETIC ACTIVITY from the SIDC # # (RWC Belgium) # #--------------------------------------------------------------------# SIDC URSIGRAM 00402 SIDC SOLAR BULLETIN 02 Apr 2010, 1252UT SIDC FORECAST (valid from 1230UT, 02 Apr 2010 until 04 Apr 2010) SOLAR FLARES : Quiet conditions (<50% probability of C-class flares) GEOMAGNETISM : Quiet (A<20 and K<4) SOLAR PROTONS : Quiet PREDICTIONS FOR 02 Apr 2010 10CM FLUX: 078 / AP: 011 PREDICTIONS FOR 03 Apr 2010 10CM FLUX: 077 / AP: 005 PREDICTIONS FOR 04 Apr 2010 10CM FLUX: 076 / AP: 003 COMMENT: Two sunspot groups on the solar disc (Catania numbers 54 and 56, NOAA ARs 1057 and 1059 respectively) are unlikely to produce a C-flare due to low X-ray background flux and its slow variability. An interplanetary shock wave was detected by ACE and SOHO/CELIAS at 06:45 UT today. The solar source of this shock is probably a CME first detected by LASCO C2 at 03:08 UT on March 30. The angular extent of the CME was around 110 degrees. It was accelerating to reach the speed of around 350 km/s in the LASCO C3 field of view. The CME originated from the eruption in the Catania sunspot group 56 (NOAA AR 1059) at S15E40 that was not associated with any reported flare. However, coronal dimmings and post-eruption loops were observed by SECCHI/EUVI onboard STEREO B starting from around 03:00 UT. Due to the position of the erupting active region away from solar central meridian and non-halo appearance of the CME, we believe that the ICME itself will probably miss the Earth. The interplanetary magnetic field (IMF) magnitude reached 7 nT in the post-shock sheath. The IMF north-south component was fluctuating, so the K index reached only 3 (as reported by IZMIRAN and NOAA) The solar wind speed and the IMF magnitude are currently back at average levels for the slow solar wind (460 km/s and 5 nT respectively). We thus do not expect any further geomagnetic disturbance in the coming hours. Catania sunspot group 56 (NOAA AR 1059) is currently situated close to the solar central meridian, so any CME originating from this group may arrive to the Earth with possible geomagnetic consequences. TODAY'S ESTIMATED ISN : 018, BASED ON 09 STATIONS. SOLAR INDICES FOR 1 Apr 2010 WOLF NUMBER CATANIA : 026 10CM SOLAR FLUX : 079 AK CHAMBON LA FORET : /// AK WINGST : 012 ESTIMATED AP : 013 ESTIMATED ISN : 017, BASED ON 16 STATIONS. NOTICEABLE EVENTS SUMMARY DAY BEGIN MAX END LOC XRAY OP 10CM RADIO BURST TYPES Catania NOAA NOTE NONE END BT #--------------------------------------------------------------------# # Solar Influences Data analysis Center - RWC Belgium # # Royal Observatory of Belgium # # Fax : 32 (0) 2 373 0 224 # # Tel.: 32 (0) 2 373 0 491 # # # # For more information, see http://sidc.be/products/meu # # Please do not reply directly to this message, but send comments # # and suggestions to 'sidctech@oma.be'. If you are unable to use # # that address, use 'rvdlinden@spd.aas.org' instead. # # To unsubscribe, visit http://sidc.be/registration/unsub.php # #--------------------------------------------------------------------#