The ARs rotating over the east limb into the visible disk are producing most of the activity at present. The strongest flare was a C4.9 with peak at 11:52 UT, originating in NOAA AR 2104 (no Catania number). This AR, and NOAA AR 2102 (no Catania number), will most likely produce more C-class and probably M-class flares.With solar wind speeds around 350 km/s and interplanetary magnetic field with a magnitude of 3 nT geomagnetic conditions are quiet and expected to remain so.
SIDC
Equipment: Coronado 90 + Imaging Source DMK + LX75
Processing: Photoshop, Avistack 300 frames
Date: 06/29/14
Time UT: 16:00
Exposure 1/500 sec.
Observatory Sponli