Recent Events Reported by Observers
Previous Next
Detected by weiliu, Submitted at 2012-05-01T01:22:14
2012-04-27T15:30:04 --> 2012-04-27T17:50:04
Two consecutive surges on the SW limb.
Detected by weiliu, Submitted at 2012-04-30T22:41:54
2012-04-28T09:00:04 --> 2012-04-28T14:00:04
A portion of a small filament near NE limb is ejected along a loop-shaped trajectory and falls back down.
Detected by weiliu, Submitted at 2012-04-30T22:31:24
2012-04-28T09:00:04 --> 2012-04-28T14:00:04
A filament erupts in SW and results in two-ribbon brightening in the chromosphere/low corona seen at 211.
Detected by weiliu, Submitted at 2012-04-27T19:58:26
2012-04-27T07:20:04 --> 2012-04-27T12:00:04
A small scale flare from AR near the NW limb.
Detected by weiliu, Submitted at 2012-04-27T19:37:50
2012-04-26T16:40:04 --> 2012-04-27T16:10:04
A polar crown prominence inside a high-latitude coronal cavity diminishes in size by mass drainage and is eventually depleted in one day. This is likely a result of imbalance between mass supply (by condensation, see e.g., Liu, Berger, Low 2012, ApJ Lett, http://adsabs.harvard.edu/abs/2012ApJ...745L..21L) and drainage. Note that the prominence does not erupt, nor does the coronal cavity (at least up to the end of the observation time window). Would this have implications for CME initiation models where mass unloading plays a role?
Detected by weiliu, Submitted at 2012-04-27T19:37:49
2012-04-26T16:40:04 --> 2012-04-27T16:10:04
A polar crown prominence inside a high-latitude coronal cavity diminishes in size by mass drainage and is eventually depleted in one day. This is likely a result of imbalance between mass supply (by condensation, see e.g., Liu, Berger, Low 2012, ApJ Lett, http://adsabs.harvard.edu/abs/2012ApJ...745L..21L) and drainage. Note that the prominence does not erupt, nor does the coronal cavity (at least up to the end of the observation time window). Would this have implications for CME initiation models where mass unloading plays a role?
Detected by halocme, Submitted at 2012-04-27T17:41:47
2012-04-23T17:00:04 --> 2012-04-23T19:00:04
The propagation is mostly southward, and the front seems to encounter several active regions. The one toward southeast appears to be a secondary wave starting at an AR. The associated CME is unimpressive.
Detected by halocme, Submitted at 2012-04-27T06:36:57
2012-04-24T07:00:04 --> 2012-04-24T09:00:04
This propagating front iis also associated with a partial halo CME observed by LASCO.
Detected by cheung, Submitted at 2014-02-10T02:14:34
2012-04-26T00:40:04 --> 2012-04-26T03:20:04
A very pretty surge with much of the material falling back down.
Detected by cheung, Submitted at 2014-02-10T02:14:34
2012-04-25T10:00:04 --> 2012-04-25T11:50:04
Some energetic event leads to a surge of material into a magnetic fan.
Detected by cheung, Submitted at 2014-02-10T02:14:27
2012-04-24T06:50:04 --> 2012-04-24T09:20:04
THIS is a tornado In this filament eruption, the filament being launched is seen to expand and unwind over Alfvenic time scales. This event is visually reminiscent of magnetically driven jets in MHD simulations of accretion disks.
Detected by halocme, Submitted at 2012-04-25T19:43:57
2010-11-15T14:20:12 --> 2010-11-15T14:59:48
Just to fill in a gap of the knowledgebase... This "coronal" wave seems to be associated with a minor electron event at L1.
Detected by cheung, Submitted at 2012-04-24T01:22:08
2012-04-23T13:00:04 --> 2012-04-23T17:30:04
In this region of cross-equatorial reconnection, there seems to be an abundance of coronal condensation in locations that may act as favorable sites of reconnection between different domains of connectivity. Perhaps turbulent reconnection creates plasmoids which trap material and facilitate coronal condensation?
Detected by cheung, Submitted at 2012-04-24T01:22:08
2012-04-23T13:00:04 --> 2012-04-23T17:30:04
In this region of cross-equatorial reconnection, there seems to be an abundance of coronal condensation in locations that may act as favorable sites of reconnection between different domains of connectivity. Perhaps turbulent reconnection creates plasmoids which trap material and facilitate coronal condensation?
Detected by cheung, Submitted at 2012-04-24T01:14:28
2012-04-21T08:30:04 --> 2012-04-21T11:10:04
This filament seems to lift off at first but then appears stuck. The filament material also fades away.
Detected by cheung, Submitted at 2012-04-24T01:11:40
2012-04-21T05:00:04 --> 2012-04-21T08:40:04
Just as this filament erupts, the moon passes by and occults the southwestern quadrant of the solar disk.
Detected by cheung, Submitted at 2012-04-24T01:07:35
2012-04-20T13:20:04 --> 2012-04-23T03:20:04
Some event from behind the limb seems to inject a large quantity of mass into the region that forms a quiescent filament. The filamentary material is clearly visible in 304 (red/orange). The morphology in the 171 channel (yellow) indicates a coronal cavity above the filament. This cavity+filament system is eventually destablized and launches off.
Detected by cheung, Submitted at 2012-04-24T01:07:35
2012-04-20T13:20:04 --> 2012-04-23T03:20:04
Some event from behind the limb seems to inject a large quantity of mass into the region that forms a quiescent filament. The filamentary material is clearly visible in 304 (red/orange). The morphology in the 171 channel (yellow) indicates a coronal cavity above the filament. This cavity+filament system is eventually destablized and launches off.
Detected by cheung, Submitted at 2012-04-24T01:04:39
2012-04-22T11:20:04 --> 2012-04-22T16:40:04
The footpoints of this filament eruption span a latitude range of almost 45 degrees.
Detected by cheung, Submitted at 2012-04-20T21:21:37
2012-04-19T18:10:04 --> 2012-04-20T04:20:04
Apparent rotational motion as the filament lifts off.
