Highest Rated Events (only 193 and 304 shown) All AR FE FL
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by berger, Submitted at 2012-01-19T22:21:12
2012-01-13T14:10:04 --> 2012-01-14T00:00:04
Small filament in quiet Sun region erupts with a very bright two-ribbon flare and subsequent post-flare loop arcade.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by berger, Submitted at 2012-01-19T22:13:53
2012-01-13T00:00:04 --> 2012-01-13T12:30:04
Single filament erupts in two places in sequence. A section of the filament still remains even after two fairly large eruptions.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-01-11T07:37:59
2012-01-05T11:00:04 --> 2012-01-05T14:00:04
One end of the filament appears to open up, and the other end grows into what looks like a surge.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-01-11T07:31:22
2012-01-05T06:30:01 --> 2012-01-05T10:00:01
The flare was of short duration, but eruptive. Note the spiky arcade see at 94 A.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-01-11T01:24:35
2012-01-04T08:30:00 --> 2012-01-04T12:00:00
In addition to two brigthenings/eruptions across the coronal hole near central meridian, at least three other regions seem to erupt around the same time (the SW eruption is quite late). The one near east limb is indicated by a box. How are some of these magnetically connected?
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-01-11T01:10:57
2012-01-04T05:10:12 --> 2012-01-04T07:40:12
Minor dimming on the NW limb appears to be contemporaneous with jet-like ejections near the NE limb. This pattern seems to repeat, suggesting the link between the two phenomena.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-01-10T23:26:40
2012-01-03T23:10:12 --> 2012-01-04T00:50:12
The minor eruption slightly west of central meridian immediately follows that on the east limb. Is this just by cosincidence?
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2012-01-06T01:06:25
2012-01-02T17:20:04 --> 2012-01-02T21:44:04
QS filament activation, without a clear sign of eruption, other than what appear as post-eruption loop arcade and flare-ribbon like features.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2012-01-06T01:03:15
2012-01-02T22:44:04 --> 2012-01-03T00:56:04
An eruption from a small AR looks like a spray/surge, but also suggests reaching the high corona if not forming a true, albeit very narrow, CME.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2012-01-06T01:00:55
2012-01-02T14:24:04 --> 2012-01-02T15:56:04
A prominence erupts from behind the W limb, displaying a complex rope-like structure, with high coronal oscillations excited in the process.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2012-01-06T01:00:53
2012-01-02T14:24:04 --> 2012-01-02T15:56:04
A prominence erupts from behind the W limb, displaying a complex rope-like structure, with high coronal oscillations excited in the process.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2012-01-06T00:07:42
2012-01-01T05:08:04 --> 2012-01-01T10:44:04
A coronal reconfiguration, reminiscent of a filament eruption, but mainly manifested because of thermal changes in the QS corona N or a small AR.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2012-01-06T00:05:33
2012-01-01T00:00:04 --> 2012-01-01T02:36:04
QS filament eruption with post-eruption loop system.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-01-02T21:55:58
2012-01-01T00:20:24 --> 2012-01-01T02:20:24
The eruption seems to be slow, although accompanying a weak two-ribbon flare (not showing up in GOES with a ~B4 background lebel). The associated CME is narrow, but it may reflect an edge-on perspective.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-01-02T21:45:44
2011-12-31T16:00:04 --> 2011-12-31T16:59:28
This concludes the series of M-class flares from AR 11389, for which the standard cartoon model of eruptive flares does not seem to apply.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-01-02T21:39:43
2011-12-31T12:50:24 --> 2011-12-31T13:40:12
This is the fourth example of confined M-class flares in AR 11389.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-01-02T21:07:44
2011-12-31T20:20:24 --> 2011-12-31T22:50:24
The filament/prominence itself is best viewed at 304 A. It pushes material ahead of it, which is captured at 211 A and 171 A as a front (in emission). This eruption was associated with a slow CME that first appeared in the LASCO C2 image at 23:12 UT.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-01-02T20:58:52
2011-12-31T20:10:24 --> 2011-12-31T22:10:24
The eruption originated from the northwestern periphery of AR 11386. No obvious pre-existing filament was seen.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-01-02T20:50:42
2011-12-31T10:40:12 --> 2011-12-31T12:10:12
This is yet another event of coronal dimming due to an eruption, following three similar events. This one is the weakest, not accompanying flares.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-01-02T20:41:41
2011-12-31T16:20:24 --> 2011-12-31T17:10:24
This may be a typical jet from an anemone region. But the base region does not seem to be as drastically reconfigured as in the cartoon model.
