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 More C-flares are possible,probability for an M-fl
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vk3pa
Deceased

Australia
1714 Posts

Posted - 22 Mar 2006 :  07:47:45 AM  Show Profile  Visit vk3pa's Homepage  Reply with Quote
Catania sunspot group 15 (NOAA AR 0862) has grown up further
and developed a beta-gamma configuration of the photospheric magnetic
field. C2.5 and C1.3 flares (peaking at 09:44 UT and 12:04 UT
respectively) occurred today in this group. More C-flares are possible,
and there is a low probability for an M-flare. The solar wind speed
decreased down to around 600 km/s and the magnetic field remains at the
average level. We expect quiet geomagnetic conditions for the next 48
hours.
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