Recent Events Reported by Observers
Previous NextDetected by cheung, Submitted at 2014-05-29T23:40:27
2014-05-18T06:10:03 --> 2014-05-18T08:40:03
Prior to the eruption the coronal rain in this region seem to outline a teardrop-shaped volume. During the eruption some of the rain material are expelled, some sucked to the lower atmosphere and perhaps the rest heated out of the 304 passband.One conjecture is that the coronal rain is outlining a quasi-separatrix layer.
Detected by cheung, Submitted at 2014-05-29T23:40:25
2014-05-18T06:10:03 --> 2014-05-18T08:40:03
Prior to the eruption the coronal rain in this region seem to outline a teardrop-shaped volume. During the eruption some of the rain material are expelled, some sucked to the lower atmosphere and perhaps the rest heated out of the 304 passband.One conjecture is that the coronal rain is outlining a quasi-separatrix layer.
Detected by cheung, Submitted at 2014-05-29T23:40:28
2014-05-16T20:10:03 --> 2014-05-16T20:40:03
Satuaration in AIA images and a pronounced diffraction pattern centered on a localized patch.
Detected by cheung, Submitted at 2014-05-29T23:40:28
2014-05-16T04:02:03 --> 2014-05-16T04:58:03
This is a very pretty example of a blow-out jet with an untwisting, erupting filament.
Detected by cheung, Submitted at 2014-05-29T23:40:24
2014-05-16T04:02:03 --> 2014-05-16T04:58:03
This is a very pretty example of a blow-out jet with an untwisting, erupting filament.
Detected by cheung, Submitted at 2014-05-29T23:40:27
2014-05-18T09:30:03 --> 2014-05-19T00:00:03
This eruption seems to squeeze a blob of field/plasma to the north
Detected by cheung, Submitted at 2014-05-23T22:40:25
2014-05-12T06:27:03 --> 2014-05-12T07:17:03
The activation causes oscillations of loops in a neighboring filament channel.
Detected by cheung, Submitted at 2014-05-23T22:40:23
2014-05-12T06:27:03 --> 2014-05-12T07:17:03
The activation causes oscillations of loops in a neighboring filament channel.
Detected by cheung, Submitted at 2014-05-23T22:40:27
2014-05-12T10:40:03 --> 2014-05-12T17:30:03
This region previously spawned two giant helical surges. This eruption seems to also have arcade loops.
Detected by cheung, Submitted at 2014-05-23T22:40:23
2014-05-12T10:40:03 --> 2014-05-12T17:30:03
This region previously spawned two giant helical surges. This eruption seems to also have arcade loops.
Detected by cheung, Submitted at 2014-05-23T22:40:21
2014-05-12T10:40:03 --> 2014-05-12T17:30:03
This region previously spawned two giant helical surges. This eruption seems to also have arcade loops.
Detected by cheung, Submitted at 2014-05-23T22:40:27
2014-05-11T17:10:03 --> 2014-05-11T18:30:03
This helical surge emanates from the same region as another helical surge that occurred earlier in the day.
Detected by cheung, Submitted at 2014-05-23T22:40:24
2014-05-10T22:50:03 --> 2014-05-11T01:30:03
This filament stops rising in the mid corona.
Detected by cheung, Submitted at 2014-05-23T22:40:27
2014-05-10T22:50:03 --> 2014-05-11T01:30:03
This helical surge has a length exceeding a couple hundred Mm.
Detected by cheung, Submitted at 2014-05-23T22:40:27
2014-05-10T10:10:03 --> 2014-05-10T10:40:03
The apparent helical motion of the jet suggests the field lines are untwisting.
Detected by cheung, Submitted at 2014-05-23T22:40:20
2014-05-10T10:10:03 --> 2014-05-10T10:40:03
The apparent helical motion of the jet suggests the field lines are untwisting.
Detected by cheung, Submitted at 2014-05-23T21:40:19
2014-05-09T23:10:03 --> 2014-05-10T05:10:03
The coronal loops seem to open up during this faint eruption.
Detected by cheung, Submitted at 2014-05-23T21:40:19
2014-05-09T23:10:03 --> 2014-05-10T05:10:03
The coronal loops seem to open up during this faint eruption.
Detected by halocme, Submitted at 2014-05-22T05:52:18
2014-05-21T00:45:35 --> 2014-05-21T03:09:35
In this eruption, the flux rope structure is seen at 304 A. The northern parts seems to reconnect with the surrounding corona, while the southern part expands radially. This eruption became the most decent CME during 19-21 May.
Detected by halocme, Submitted at 2014-05-22T05:52:17
2014-05-21T00:45:35 --> 2014-05-21T03:09:35
In this eruption, the flux rope structure is seen at 304 A. The northern parts seems to reconnect with the surrounding corona, while the southern part expands radially. This eruption became the most decent CME during 19-21 May.