Solar flare measuring M1.7 erupted on November 8, 2012 at 02:23 UTC. The source of this event is newly formed region rotating into view, Region 1611 (N12E66). The event started at 02:28, peaked at 02:23 and ended at 02:25 UTC. Type II Radio Emission was recorded
The Sun produced a series of at least eight coronal mass ejections (CMEs) over a two-day period (November, 2-4, 2012). Some of them overlapped each other as the Sun burst some of them into space in a rapid-fire style. The series was taken by the STEREO Ahead spacecraft
Magnetic filament eruption took place beyond the western limb, producing a halo or partial-halo CME on November 3. In fact, three CME clouds were ejected into space, with one appeared to have slight chance to become geoeffective. Minor solar wind stream from
The video by Solar Dynamics Observatory (SDO) combines three wavelengths with similar temperatures, highlighting different parts of the solar corona showing the Sun from September 1 through September 30, 2012. The start of the Fall Eclipse Season could be seen, when
Solar activity was at low levels for the past 24 hours and X-Ray flux plot shown merely C-class threshold. However, a prominence eruption was observed north of Region 1600.A bright CME was observed in STEREO Ahead COR 2 imagery at 18:24 UTC on October 27. Latest
X1.8 solar flare peaked at 03:17 UTC on October 23, 2012 around Active Region 1598, which is still several days away from directly facing Earth from center disk. NOAA/SWPC forecasters estimated 20% chance for another X-class event.Space Weather Message Code:
A moderate solar flare reaching M5.06 took place at 18:51 UTC on October 22, 2012. The responsible Region was again 1598. The event started at 18:38, peaked at 18:51 and ended at 19:01 UTC.Space Weather Message Code: SUMXM5Serial Number: 99Issue Time: 2012 Oct 22
A moderate solar flare peaking at M1.38 erupted from emerging Region 1598 on October 21, 2012. This latest M-class eruption started at 19:46, peaked at 20:03 and ended at 20:20 UTC. Region 1598 was the source of yesterdays strong M9 solar flare and is moving into more
A strong solar flare reaching M9.0 took place at 18:14 UTC on October 20, 2012. Sunspot that produced it is rotating into view off the eastern limb. Associated was Type II Radio Emission. Estimated velocity was 516 km/s. Coronal mass ejection (CME) was associated but
Dozens of loops gyrated above several active regions as they were rotating into view (Oct. 13 – 17, 2012). When viewed in extreme ultraviolet light, the dancing loops of competing and connecting magnetic field lines become visible. Two minor eruptions can be observed
