Recent Events Reported by Observers
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Detected by cheung, Submitted at 2014-01-07T00:21:29
2014-01-04T15:00:03 --> 2014-01-04T17:00:03
This confined eruption emanates from the northern edge of AR 11944. The eruption instigates transverse loop oscillations.
Detected by cheung, Submitted at 2014-01-07T00:21:29
2014-01-04T15:00:03 --> 2014-01-04T17:00:03
This confined eruption emanates from the northern edge of AR 11944. The eruption instigates transverse loop oscillations.
Detected by halocme, Submitted at 2014-01-06T15:37:57
2014-01-06T07:30:35 --> 2014-01-06T08:59:23
The eruption should be from a far-side region since there is hardly an increase in GOES soft X-ray flux. A bright prominence eruption, dimming and loop oscillations are clearly seen. This is associated with a proton event that extends to > 100 MeV (thanks, Sam, for reporting this.)
Detected by halocme, Submitted at 2014-01-06T15:37:56
2014-01-06T07:30:35 --> 2014-01-06T08:59:23
The eruption should be from a far-side region since there is hardly an increase in GOES soft X-ray flux. A bright prominence eruption, dimming and loop oscillations are clearly seen. This is associated with a proton event that extends to > 100 MeV (thanks, Sam, for reporting this.)
Detected by halocme, Submitted at 2014-01-06T15:37:55
2014-01-06T07:30:35 --> 2014-01-06T08:59:23
The eruption should be from a far-side region since there is hardly an increase in GOES soft X-ray flux. A bright prominence eruption, dimming and loop oscillations are clearly seen. This is associated with a proton event that extends to > 100 MeV (thanks, Sam, for reporting this.)
Detected by halocme, Submitted at 2014-01-06T15:37:54
2014-01-06T07:30:35 --> 2014-01-06T08:59:23
The eruption should be from a far-side region since there is hardly an increase in GOES soft X-ray flux. A bright prominence eruption, dimming and loop oscillations are clearly seen. This is associated with a proton event that extends to > 100 MeV (thanks, Sam, for reporting this.)
Detected by halocme, Submitted at 2014-01-06T05:10:47
2013-12-31T09:45:35 --> 2013-12-31T12:45:35
This flare was slightly limb occulted. The dimming is seen above the flare loops. This immediately became a bright and fast (~1000 km s-1) CME. The top of some of these loops shows hot plasma in 193 A channel, above which downflows are indicated as they are in certain eruptive flares.
Detected by halocme, Submitted at 2014-01-06T05:10:46
2013-12-31T09:45:35 --> 2013-12-31T12:45:35
This flare was slightly limb occulted. The dimming is seen above the flare loops. This immediately became a bright and fast (~1000 km s-1) CME. The top of some of these loops shows hot plasma in 193 A channel, above which downflows are indicated as they are in certain eruptive flares.
Detected by halocme, Submitted at 2014-01-06T04:54:28
2013-12-30T19:45:35 --> 2013-12-30T22:45:35
There are two episodes of eruption. First, multiple loops interacted in the eastern part of the region, leading to an eruption. The second episode seems to be more straightforward, and the eruption is faster. These are very diffuse and difference movies are needed to see them. Part of the motions may represent waves rather than mass motions.
Detected by halocme, Submitted at 2014-01-06T04:42:15
2013-12-30T10:40:11 --> 2013-12-30T12:40:11
The motion toward south is noted only in difference images because it is too diffuse in intensity images. There is no clear filament eruption in 304 A or 211 A channel. Perhaps we are looking at a wave rather than a mass motion.
Detected by halocme, Submitted at 2014-01-06T04:33:09
2013-12-29T01:40:11 --> 2013-12-29T04:40:11
In difference images in these channels, we note four eruptions in three hours. First, a small eruption in the eastern hemisphere, like E50, and another one in the northen hemisphere, like N40. Then bigger ones near the southwast limb and over the west limb.
Detected by halocme, Submitted at 2014-01-06T04:33:08
2013-12-29T01:40:11 --> 2013-12-29T04:40:11
In difference images in these channels, we note four eruptions in three hours. First, a small eruption in the eastern hemisphere, like E50, and another one in the northen hemisphere, like N40. Then bigger ones near the southwast limb and over the west limb.
Detected by anny, Submitted at 2014-01-03T23:19:25
2013-12-10T00:00:03 --> 2013-12-11T00:00:03
A small dipole rapidly grows in size and eventually reconnects with the field of a nearby larger AR, judging by the formation of the 171A loops interconnecting the two.
Detected by anny, Submitted at 2014-01-03T23:11:07
2013-12-09T00:00:03 --> 2013-12-10T00:00:03
A small dipole emerges in a region surrounded by three large AR's. Some loops connecting it with the W-most large AR can be seen relatively early.
Detected by anny, Submitted at 2014-01-03T23:06:49
2013-12-09T14:14:03 --> 2013-12-09T20:28:03
A small prominence resides on the NE limb for at least half a day, and a faint small cavity can be seen on its top. Eventually, perhaps disturbed by the activity in the nearby AR, the cavity takes off, while the prominence does not seem to follow along, it falls down to the surface as a coronal rain.
Detected by anny, Submitted at 2014-01-03T23:06:49
2013-12-09T14:14:03 --> 2013-12-09T20:28:03
A small prominence resides on the NE limb for at least half a day, and a faint small cavity can be seen on its top. Eventually, perhaps disturbed by the activity in the nearby AR, the cavity takes off, while the prominence does not seem to follow along, it falls down to the surface as a coronal rain.
Detected by anny, Submitted at 2014-01-03T23:01:54
2013-12-09T10:32:03 --> 2013-12-09T12:54:03
A small filament at the core of an AR on the E disk erupts forming an extended surge off the limb.
Detected by anny, Submitted at 2014-01-03T22:54:28
2013-12-08T19:42:03 --> 2013-12-09T00:00:03
A small bubble (bright in 304A) is ejected from an AR at the E disk. This bubble travels along the nearby filament-like structure, gradually increasing in size, then goes past the dark 304A structure, lifts up along what appears a spiral trajectory, and falls down over an extended patch in the quiet sun as coronal rain.
Detected by anny, Submitted at 2014-01-03T22:50:05
2013-12-08T03:12:03 --> 2013-12-08T07:58:03
A small filament eruption on the W limb. A faint cavity forms at the onset of eruption and appears to erupt as well.
Detected by schryver, Submitted at 2014-10-14T22:18:09
2014-01-02T09:04:03 --> 2014-01-02T11:32:03
A near-equatorial QS filament erupts from near the W limb. Synchronously, an AR filament near DC activates, as does a filament SE of the primary eruption. A fragment of a prominence to the S of the eruption exhibits briefly oscillations.
