AR3664 has produced its most powerful flare yet, peaking at X5.9, accompanied by significant dimming and a coronal wave. This marks the second strongest flare of SC25.
The X2.9 flare was accompanied by large dimming and a coronal wave. Nice CME was launched, not an Earth-directed. Hopefully, AR3664 will maintain its active streak for more potential flares in this second round.
M9.7 flare produced an energetic halo CME, causing an S2-level radiation storm. CME is mainly directed to the west. Glancing impact is expected on June 10th.
AR3664 isn't done yet. Produced a long-duration M6.6 flare, resulting in a fast, full halo CME. The bulk of the CME is directed to the SW, with an Earth directed component. Impact is expected on May 15th.
AR3664 has produced its 11th and strongest X-flare, with an intensity of X8.7. This event was followed by an eruptive M4.4 flare from the incoming sunspot AR3682 on the NE limb. Both CMEs are not Earth-directed.
The X3.9 flare from AR3664 accompanied by large dimming, has launched its 6th halo CME. Bulk of the CME is heading westward. CME shockwave is expected on May 13th.
Before the X5.8 flare, a filament erupted at the disk center in the southern hemisphere, producing a faint partial halo CME. 2nd CME is associated with the X5.8 flare, is mainly moving westward. Expect the shockwave on May 12-13th. 3rd CME originated from behind the NE limb.
Three halo CMEs were seen in LASCO imagery. 1st CME visible at 04:41 UTC, is related to the farside eruption. 2nd CME visible from 05:33 UTC, is associated with an M4.2 flare from AR3766. 3rd CME visible at 06:33 UTC, resulted from an M3.1 flare in AR3762.
Double X-flare! An eruptive X1.7 flare occurred in AR3767 on the SW limb at 13:40 UTC, followed by an impulsive X1.1 flare from AR3780 in the SE at 15:27 UTC.
An eruptive M8.6 flare occurred in AR3664 at 12:04 UTC, resulting in another full halo CME directed towards Earth. We are now expecting two strong impacts on May 10-11.
An eruptive M9.9 flare occurred in AR3766 near the center disk, accompanied by a nice coronal wave and dimming. Another Earth-directed halo CME is likely.
An X1.3 flare erupted from AR3777 at 19:35 UTC, resulting in a halo CME. The bulk of the CME was directed towards the south, with a glancing impact expected on Aug 11th.
Sunspot region AR3363 unleashed two spectacular solar flares. The first flare, an M2.7, occurred at 22:55 UTC, followed by a long-lasting M5.8 flare. These intense solar flares resulted in an S2-level radiation storm.
A large solar eruption has taken place on the far side of the sun, likely originating from AR3363, resulting in an impressive halo CME and a minor proton event.
Sunspot AR3575 continues its fiery action on the far side, unleashing another significant flare. Nice halo CME has been launched.
@halocme
@GoroDaisuki09
Three CMEs were visible in LASCO imagery. 1st CME emerged from an eruption behind the NE limb; the 2nd CME originated from AR3575 on the far side; and the 3rd CME resulted from a filament eruption in the NW quadrant.
A filament eruption with a nice dimming effect occurred in the southwest quadrant of the Sun, resulting in a CME that is mostly heading southward. The eastern part of the CME is expected to impact on April 27th.
An interesting eruption has occurred on the Earth-facing solar disk. A C7.1 flare from ARs 3285/3288 was followed by a two-ribbon flare in the disk center. CME has been launched and is headed towards Earth, with an expected impact on May 1-2.
Solar activity continues to intensify. An eruptive M8.7 flare occurred in AR3762, followed by a long-duration M4.2 flare from AR3766 and the incoming region on the SE limb. Additionally, a filament erupted on the SW limb.
Another strong X-flare event has occurred in sunspot AR3386, reaching its peak at X1.5. Proton levels have increased and returned to the S1 radiation storm threshold.
A strong solar eruption has occurred on the far-side of the sun, accompanied by a widespread movement of coronal dimming. Large CME can be observed on LASCO C2 imagery. Not an Earth-directed.
Filament eruption was observed near AR3803, with the resulting CME directed to the NE. This was followed by a large eruption from behind the NW limb, produced a partial halo CME.
Two large farside eruptions occurred: 1st, likely a filament eruption with dimming over the north pole, produced a slow CME. 2nd, from behind the NE limb related to a long-duration M-flare, generated a partial halo CME. Note: Sun-diving comet is entering C3 at 4 o'clock position.
Two CMEs are visible in LASCO imagery. The CME resulting from the filament eruption is mainly directed northward, followed by a partial halo CME likely associated with a farside eruption.
Multiple CMEs were observed in LASCO C2 imagery over the last 24 hours, associated with prominence and far-side eruptions. None are considered geoeffective. A small filament eruption was observed below AR3672 around 04:15 UTC, and the resulting CME is directed northeast.
Two filament eruptions were observed. 1st eruption occurred in the NW quadrant and did not produce a CME. Followed by the eruption of a larger filament located in the SW quadrant. M1.1 post-flare loop continued to grow behind the SW limb.
Double eruption! 1st eruption was a spectacular event that occurred on the northeastern limb, followed by a 2nd eruption from behind the northwest limb.
Another filament eruption occurred in the SW quadrant, resulting in a partial halo CME. The CME is mainly directed south, with a glancing impact expected on July 3rd.
A long-duration M4.2 flare occurred in AR3296, resulting in an energetic halo CME expected to impact on May 11th. Shortly after, an M5.0 flare occurred, which was not a remarkable occurrence.
Filament eruption occurred near the disk center in the southern hemisphere, accompanied by a double ribbon flare. The resulting CME was primarily directed towards the south. Impact is expected on March 19th due to the location of the eruption.
An M3.1 flare occurred in the sunspot AR3372, followed by an M1.0 from AR3373. Simultaneously, a farside eruption was observed behind the SW limb. CME resulting from the M3.1 flare appeared faint, while the farside event produced a bright CME.
A sequence of eruptions has taken place in the northeast quadrant, beginning with a prominence eruption, followed by a C9.5 flare from AR3297, and a long-duration M2.1 flare from AR3296.
Yesterday's filament eruption produced a faint halo CME that became visible on LASCO C2 imagery at 19:10 UTC. It was difficult to observe due to overlapping with the previous partial halo CMEs. Impact is likely to occur on July 17-18.
A strong X1.1 eruptive flare occurred in sunspot AR3614, accompanied by a large dimming and a coronal wave. Simultaneously, sunspot AR3615 also produced flaring activity, likely at the M-class level.
An impressive filament eruption occurred near AR3370 in the southeastern region around 18:40 UT. This eruption was accompanied by a C8.9 flare and expelled a substantial amount of material. Additionally, multiple CMEs were observed on both sides of the Sun's limb.
A filament eruption was observed in association with a long-duration M1.6 flare from sunspot AR3386. It produced a bright CME and caused an S1 level radiation storm. Also, an M2.1 flare was detected from AR3380 behind the western limb.
AR3664 continues its intense activity, producing a major X-flare peaking at X3.4. Currently located behind the limb, therefore CME no threat to Earth. However, keep an eye on proton levels. Also, a filament eruption with dimming occurred in the NE quadrant.
Geomagnetic storm has escalated to a Severe G4 level!
ALERT: Geomagnetic K-index of 8, 9-
Threshold Reached: 2024 Jun 28 1415 UTC
Synoptic Period: 1200-1500 UTC
NOAA Scale: G4 - Severe
Impressive! Sunspot AR3575 continues to produce major flares on the far-side, launched another halo CME. Additionally, a minor eruption occurred on the NE limb.
Widespread coronal dimming was observed at the south pole around 03:55 UT, indicating that sunspot AR3575 has produced another major eruption on the far side. Halo CME was launched, with proton levels once again on the rise.
Recently, two eruptions were recorded. An eruptive C8.9 flare from AR3360 with an eastward-directed CME, followed by a filament eruption near AR3359, causing a partial halo CME moving southeast. A chance of glancing impact on July 7th.
Another strong M-flare occurred in sunspot region AR3435, peaking at M8.7. The associated CME is mainly directed to the SE, with the possibility of a glancing impact on Sep 24. Followed by a large prominence eruption behind the NE limb, resulting in a bright CME.