Survey Results: Difference between revisions
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*[http://www.lmsal.com/hek/hcr?cmd=view-event&event-id=ivo%3A%2F%2Fsot.lmsal.com%2FVOEvent%23VOEvent_IRIS_20160409_180221_3660259503_2016-04-09T18%3A02%3A212016-04-09T18%3A02%3A21.xml IRIS] | *[http://www.lmsal.com/hek/hcr?cmd=view-event&event-id=ivo%3A%2F%2Fsot.lmsal.com%2FVOEvent%23VOEvent_IRIS_20160409_180221_3660259503_2016-04-09T18%3A02%3A212016-04-09T18%3A02%3A21.xml IRIS] | ||
Some detailed features in the whole event: | Some detailed features seen from dynamic spectrum in the whole event: | ||
{| class="wikitable" | {| class="wikitable" | ||
!scope="col" width="150" | Time | !scope="col" width="150" | Time | ||
!scope="col" width="150" | Pkot | |||
!scope="col" width="150" | | |||
!scope="col" width="1050" | Description | !scope="col" width="1050" | Description | ||
|- | |- | ||
|19:43~19:44 UT | |19:43~19:44 UT | ||
|Few stripes at lower frequency | |Few stripes at lower frequency | ||
| | | | ||
|- | |- | ||
|20：08~20：10 UT | |20：08~20：10 UT | ||
|Type III like features at lower frequency and Gyrosynchrotron emission at higher frequency | |Type III like features at lower frequency and Gyrosynchrotron emission at higher frequency | ||
| | | | ||
|- | |- | ||
Revision as of 02:41, 13 October 2017
VLA Survey Results.
You can upload your VLA survey results here and I set the 2016Feb18 event as an example.
2016 Feb 18
Summary for whole event:Including C-class flare,Coord with Hinode and IRIS (HOP 297); Limb eruptive flare.File:20160218 sum.png or go to Prof. Chen's page to see the summary.
Some detailed features seen from dynamic spectrum in the whole event:
| Time | Pkot | Description | |
|---|---|---|---|
| 19:43~19:44 UT | Few stripes at lower frequency | ||
| 20：08~20：10 UT | Type III like features at lower frequency and Gyrosynchrotron emission at higher frequency | ||
| 21:09~21:12 UT | Pulsation Features | File:2110.png | From the Rhessi image, we can see the features in dynamic spectrum is corresponding to the sudden rising at 3-25keV and from the AIA image,it seems the source locates at the foot of a loop. |
Below are some movies for this event
| Dynamic spectrum | |
|---|---|
| AIA Full sun | |
| Action Region 12501 | |
| Action Region 12497 |
2016-Feb-19
Summary for whole event:
Some detailed features in the whole event:
| Time | Features | Plot | Description |
|---|---|---|---|
| @ UT | |||
| @UT | |||
| @UT |
Below are some movies for this event
| Dynamic spectrum | |
|---|---|
| AIA Full sun | |
| Action Region 1 | |
| Action Region 2 |
2016-Apr-09
Summary for whole event:
Some detailed features in the whole event:
| Time | Features | Plot | Description |
|---|---|---|---|
| @ UT | |||
| @UT | |||
| @UT |
Below are some movies for this event
| Dynamic spectrum | |
|---|---|
| AIA Full son | |
| Action Region 1 | |
| Action Region 2 |