The solar flaring activity was at low levels with several C-class flares being detected in the last 24 hours. The largest flare was a C6.3 flare, peaking at 09:14 UTC on June 06, associated with NOAA AR 3327 (beta class). This region was the main driver of the flaring activity over the past 24 hours. Isolated C-class flaring was produced by NOAA AR 3315 and NOAA AR 3317 from behind the west limb. NOAA AR 3323 (beta-gamma class) remains the largest and most complex active region on the visible solar disc but remained quiet. NOAA AR 3327 (beta class) is the second largest region on the visible disc. It has developed more trailing spots and enlarged its area, but has been silent. Other regions on the disc have simple configuration of their photospheric magnetic field (alpha and beta) and did not show any significant flaring activity. The solar flaring activity is expected to remain at low levels, with C-class flares likely and a chance for M-class flares.
No Earth-directed coronal mass ejections (CMEs) were detected in the available coronagraph imagery.
Over the past 24 hours the greater than 10 MeV GOES proton flux was at nominal levels and is expected to remain so over the next days.
The greater than 2 MeV electron flux was below the 1000 pfu threshold and is expected to remain below this threshold for the
next days.The 24h electron fluence was at normal level. The electron fluence is expected to be at normal levels in the next days.