M3.9 and M1.5 solar flares erupt from AR 3112
An impulsive M3.9 solar flare erupted from Active Region 3112 Beta at 08:42 UTC. The flare started at 08:36 and ended at 08:46 UTC. It was followed by M1.5 at 10:52 UTC from the same region.

An impulsive M3.9 solar flare erupted from Active Region 3112 Beta at 08:42 UTC. The flare started at 08:36 and ended at 08:46 UTC. It was followed by M1.5 at 10:52 UTC from the same region.

A major solar flare, measuring X1.0 at its peak at 20:25 UTC, erupted on October 2, 2022, from Active Region 3110. The event started at 19:53 and ended at 20:34 UTC.

A strong solar flare, measuring M8.7 at its peak, erupted from Active Region 3110 at 02:21 UTC on October 2, 2022. The event started at 02:08 and ended at 02:21 UTC. The event comes several hours after impulsive M5.8 from the same region at 20:10 UTC on October 1.

A strong M7.9 solar flare erupted from Active Region 3098 at 09:49 UTC on September 16, 2022. The event started 09:44 and ended at 09:56 UTC.

A spectacular full-halo coronal mass ejection (CME) erupted on the farside of the Sun on September 5, 2022. The source is Active Region 3088, which is expected to return to Earth’s view in about a week.

Active Region 3089 (Beta) produced three M-class solar flares on August 26, 2022 – M2.1 at 10:55 UTC, M7.2 at 12:14 UTC, and M5.3 at 12:31 UTC.

A G2 – Moderate geomagnetic storm watch is in effect for August 18, 2022, as a result of CME activity on August 14 and 15 coupled with a recurrent, negative polarity CH HSS.

A long-duration C5.6 solar flare erupted from Active Region 3060 at 01:11 UTC on July 21, 2022, generating an impressive Earth-directed coronal mass ejection (CME).

A G1-Minor geomagnetic storm watch is in effect for July 21, 22 and 23, 2022 as a result of slow-moving coronal mass ejection (CME) coupled with negative polarity coronal hole high speed stream (CH HSS).

A long-duration M2.5 solar flare erupted from AR 3053 at 20:49 UTC on July 8, 2022, producing a partial halo coronal mass ejection (CME).