Survey Results: Difference between revisions

From EOVSA Wiki
Jump to navigation Jump to search
Line 4: Line 4:
== 2016 Feb 18 ==
== 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.
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.
*[http://darts.isas.jaxa.jp/solar/hinode/query.php?coA=basic&fgA=basic&spA=basic&xrA=basic&eiA=basic&coB=&coC=&coD=&coE=&coF=&coG=1&coH=&coI=&coJ=&coK=&coL=&coM=&coN=&coO=&coP=&coQ=&fgD=&fgL=&fgM=&fgN=&fgO=&fgP=&fgQ=&fgR=&fgS=&fgT=&spD=1&spE=&spF=&spG=&spH=&spI=&spJ=&spK=&spL=&spM=&spN=&spO=&spP=&spQ=&spR=&spS=&spT=&spU=&spV=&xrE=&xrF=&xrG=&xrH=&xrJ=&xrK=&xrL=&xrM=&xrN=&xrO=&xrP=&xrQ=&xrR=&eiE=&eiF=&eiG=&eiH=&eiJ=&eiK=&eiL=&eiN=&eiO=&eiP=&eiQ=&eiR=&eiS=&A19=Search&inst%5B%5D=fg&inst%5B%5D=sp&inst%5B%5D=xr&inst%5B%5D=ei&plot=no&tmSY=2016&tmSM=02&tmSD=18&tmSh=18&tmSm=00&tmEY=2016&tmEM=02&tmED=19&tmEh=00&tmEm=00&posX=&posY=&posrX=&posrY=&max=1000&fgB%5B%5D=0&fgE=0&fgG=&fgH=&fgI=&fgJ=&spB%5B%5D=0&xrB%5B%5D=0&eiB%5B%5D=0 Hinode]


Some detailed features in the whole event:
Some detailed features in the whole event:

Revision as of 02:34, 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 in the whole event:

Time Features Plot 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 son
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