Growing Sunspot 1402 erupted in morning of January 23, 2012 around 04:00 UTC, producing a long-duration M8.7 solar flare. Each category for x-ray flares (B,C,M,X) has nine subdivisions ranging from C1 to C9, M1 to M9, and X1 to X9. This one ranks M9, which is only
A strong solar flare reaching M8.7 was generated by Sunspot 1402 in the northern hemisphere. The flare peaked at 03:59 UTC monday morning (Jan 23 2012) and started off an a long duration M1.0 event (LDE) before eventually rising again to its maximum. An R2 Radio
A coronal mass ejection (CME) hit Earth’s magnetic field at 06:17 UTC on January 23, 2012 and produce geomagnetic storm (Kp5/G1 Level geomagnetic storm is currently in progress) and ongoing auroras around polar cycle. According to analysts at the Goddard Space Weather
A solar wind stream is buffeting Earth’s magnetic field and this is causing geomagnetic storm. A coronal mass ejection (CME) The Coronal Mass Ejection (CME) reported on Jan 19, finally impacted our geomagnetic field with a glancing blow early this morning.hit
NOAA/SWPC have determined that the CME from Active Region 1402 near disk center from the latest M3 solar flare will likely pass above (north) of Earth. This glancing blow will cause just G1 (Minor) Geomagnetic Storm activity. We can expect first signs starting from
The long-duration blast at active region 1402 produced M3.2 solar flare and CME which is heading toward Earth. This was two-wave flare and first CME wave was overtaken by the 2nd wave due to its higher speed velocity.The major bulk of the plasma cloud appears to be
Recently formed sunspot 1401 awoke yesterday afternoon and produced an M1.7 solar flare at 19:12 UTC. AR 1401 has a Beta-Gamma magnetic configuration which could lead to further solar flares. NOAA forecasters estimate a 15% to 20% chance of polar geomagnetic storms
A very long in duration C6.4 event was detected around Sunspot 1402 in the northeast quadrant. A Coronal Mass Ejection (CME) was produced, but is directed to the north and east. Most of the magnetic activity in this event appears to be above the actual
The dark vertical coronal hole, about 120,000 km wide and more than a million km long, stretches in the center of the Sun. A solar wind stream flowing from the indicated coronal hole should reach Earth on Jan. 16-17, possibly sparking auroras at
NASA’s STEREO-Behind spacecraft observed a significant eruption on the farside of the sun today. Although the blast was eclipsed by the edge of the solar disk, it nevertheless produced a long-duration C3 solar flare detectable from Earth. The blast site is not far
