Recent Events Reported by Observers
Previous NextDetected by halocme, Submitted at 2013-10-09T15:25:26
2013-10-06T13:00:03 --> 2013-10-06T17:00:03
This may not look like a major eruption. It is associated with a modest C1.1 LDE. However, it is associated with the only halo CME during the interval that can be responsible for the moderate storm that started late on 8 October 2013 (KP=5). The CME is quite diffuse with the northern part being more visible in spite of the location of the eruption (AR 1859, a good number for a geoeffective event). There is no clear filament eruption in 304 A images.
Detected by halocme, Submitted at 2013-10-09T15:25:25
2013-10-06T13:00:03 --> 2013-10-06T17:00:03
This may not look like a major eruption. It is associated with a modest C1.1 LDE. However, it is associated with the only halo CME during the interval that can be responsible for the moderate storm that started late on 8 October 2013 (KP=5). The CME is quite diffuse with the northern part being more visible in spite of the location of the eruption (AR 1859, a good number for a geoeffective event). There is no clear filament eruption in 304 A images.
Detected by halocme, Submitted at 2013-10-07T15:12:26
2013-10-05T04:00:03 --> 2013-10-05T08:00:03
The eruptive signatures are clearly noted in AIA images even though the source region is estimated to be more than 30 degrees behind the limb. The event is associated with a type II radio burst (both metric and DH), and a halo CME. Based on the LASCO MVI files archived at NRL (no movies available at GSFC because of the goverment shutdown), the bright CME is first observed at 07:10 (at the heliocentric distance of 2.8-2.9 Rs and PA of 125 deg), and the linear speed is only about 630 km/s using five difference images.
Detected by halocme, Submitted at 2013-10-07T15:12:25
2013-10-05T04:00:03 --> 2013-10-05T08:00:03
The eruptive signatures are clearly noted in AIA images even though the source region is estimated to be more than 30 degrees behind the limb. The event is associated with a type II radio burst (both metric and DH), and a halo CME. Based on the LASCO MVI files archived at NRL (no movies available at GSFC because of the goverment shutdown), the bright CME is first observed at 07:10 (at the heliocentric distance of 2.8-2.9 Rs and PA of 125 deg), and the linear speed is only about 630 km/s using five difference images.
Detected by halocme, Submitted at 2013-10-07T15:12:24
2013-10-05T04:00:03 --> 2013-10-05T08:00:03
The eruptive signatures are clearly noted in AIA images even though the source region is estimated to be more than 30 degrees behind the limb. The event is associated with a type II radio burst (both metric and DH), and a halo CME. Based on the LASCO MVI files archived at NRL (no movies available at GSFC because of the goverment shutdown), the bright CME is first observed at 07:10 (at the heliocentric distance of 2.8-2.9 Rs and PA of 125 deg), and the linear speed is only about 630 km/s using five difference images.
Detected by weiliu, Submitted at 2013-10-01T23:51:21
2013-09-30T17:30:03 --> 2013-09-30T18:40:03
An interesting surge with part of it following a loop-shaped trajectory (likely guieded by coronal loops), and another part of it returning along the original path of ascent close to the local vertical.
Detected by weiliu, Submitted at 2013-10-01T23:38:22
2013-09-29T20:30:03 --> 2013-09-30T00:00:03
A large filament between two ARs erupts, producing nice two-ribbon brightenings. It does not seem to produce an EIT wave, probably because of its gradual (rather than impulsive) acceleration profile.
Detected by weiliu, Submitted at 2013-10-01T23:27:11
2013-09-29T10:40:03 --> 2013-09-29T12:10:03
A surge likely associated with a behind-the-limb eruption on the east limb. Note the wavy trajectory of the ejected material.
Detected by weiliu, Submitted at 2013-10-01T23:23:21
2013-09-29T00:00:03 --> 2013-09-29T02:50:03
A small eruption near the SE limb.
Detected by weiliu, Submitted at 2013-10-01T23:19:40
2013-09-29T00:00:03 --> 2013-09-30T00:00:03
A ploar-crown prominence slowly lifts off, the 171 loops and likely a coronal cavity erupted, leaving behind the 304 prominence material falling back.
Detected by derosa, Submitted at 2013-10-01T00:40:14
2013-09-28T08:00:03 --> 2013-09-28T12:00:03
Two small and not-really-very exciting filament activations on/near the east limb are notable only for the fact they are nearly simultaneous. I leave open the question as to whether they are causally related.
Detected by halocme, Submitted at 2013-10-01T00:10:46
2013-09-29T21:00:35 --> 2013-09-29T23:59:59
Someone asked the space weather forum if the Sun is dead, but this is the first major eruption in weeks. As expected, a halo CME is associated. LASCO saw its first sign at 22:12 UT. It is probably Earth-directed, and several heliospheric predictions will be made. The associated flare is C1.2.
Detected by halocme, Submitted at 2013-10-01T00:10:46
2013-09-29T21:00:35 --> 2013-09-29T23:59:59
Someone asked the space weather forum if the Sun is dead, but this is the first major eruption in weeks. As expected, a halo CME is associated. LASCO saw its first sign at 22:12 UT. It is probably Earth-directed, and several heliospheric predictions will be made. The associated flare is C1.2.
Detected by halocme, Submitted at 2013-10-01T00:10:44
2013-09-29T21:00:35 --> 2013-09-29T23:59:59
Someone asked the space weather forum if the Sun is dead, but this is the first major eruption in weeks. As expected, a halo CME is associated. LASCO saw its first sign at 22:12 UT. It is probably Earth-directed, and several heliospheric predictions will be made. The associated flare is C1.2.
Detected by schryver, Submitted at 2013-09-25T21:13:07
2013-09-24T18:36:03 --> 2013-09-25T00:00:03
A quiet-Sun filament/prominence erupts over the NE limb, with prominent post-eruption emission following ribbon expansion.
Detected by schryver, Submitted at 2013-09-25T21:10:46
2013-09-24T03:04:03 --> 2013-09-24T11:32:03
QS prominence over the SE limb at high latitude erupts. View interrupted by Earth occultation.
Detected by schryver, Submitted at 2013-09-25T21:06:29
2013-09-23T22:04:03 --> 2013-09-24T00:00:03
Compact eruption from QS with coronal dimmings in adjacent QS corona.
Detected by schryver, Submitted at 2013-09-25T21:04:41
2013-09-23T07:00:03 --> 2013-09-23T13:28:03
Quiet-Sun filament eruption from the SW quadrant.
Detected by halocme, Submitted at 2013-09-23T23:10:47
2013-09-22T18:00:03 --> 2013-09-22T19:20:03
The eruption is most clearly seen in 304 A images. The lack of obvious brightening (e.g., flare) suggests that this is energetically minor. No obvious CME is associated.
Detected by halocme, Submitted at 2013-09-23T23:10:46
2013-09-22T18:00:03 --> 2013-09-22T19:20:03
The eruption is most clearly seen in 304 A images. The lack of obvious brightening (e.g., flare) suggests that this is energetically minor. No obvious CME is associated.