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="350" | Features                           
!scope="col" width="150" | Pkot                                             
!scope="col" width="150" | Plot                 
!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