This page (revision-9) was last changed on 27-Mar-2020 14:38 by Peter Young

This page was created on 24-Feb-2010 18:22 by PeterYoung

Only authorized users are allowed to rename pages.

Only authorized users are allowed to delete pages.

Page revision history

Version Date Modified Size Author Changes ... Change note
9 27-Mar-2020 14:38 1 KB Peter Young to previous
8 07-Dec-2016 14:14 1 KB Peter Young to previous | to last
7 04-Aug-2010 21:41 2 KB PeterYoung to previous | to last
6 07-Jul-2010 20:01 2 KB PeterYoung to previous | to last
5 07-Jul-2010 19:47 1 KB PeterYoung to previous | to last
4 07-Jul-2010 19:36 1 KB PeterYoung to previous | to last
3 24-Feb-2010 22:20 1 KB PeterYoung to previous | to last
2 24-Feb-2010 18:22 1 KB PeterYoung to previous | to last
1 24-Feb-2010 18:22 2 bytes PeterYoung to last

Page References

Incoming links Outgoing links

Version management

Difference between version and

At line 1 added 3 lines
[{ALLOW edit EISMainUsers}]
[{ALLOW view Anonymous}]
!!!Worksheet 3 - Reading and browsing data
At line 5 added 52 lines
Following on from Worksheet 2, you can now read the EIS FITS file from the command line:
{{{
IDL> data=obj_new(‘eis_data’,filename)
}}}
data is an IDL object. Information is extracted from the object through a large number of ''methods'' and some examples are given below.
To determine the coordinates of the center of the raster, do:
{{{
IDL> xcen=data->getxcen(/raster)
IDL> ycen=data->getycen(/raster)
}}}
To find the exposure time for each exposure of the raster, do:
{{{
IDL> exp=data->getexp()
}}}
A single data window can be extracted by doing:
{{{
IDL> wd=data->getvar(195.12)
}}}
where the specified wavelength is used to pick out the data window containing that particular wavelength. The first dimension of WD is always wavelength, the second is always solar-Y, and the third can be either solar-X or time depending if the observation was a raster or a sit-and-stare observation.
A complete list of methods is obtained by doing
{{{
IDL> data->display_methods
}}}
while more [detailed information on some methods|EISmethods] is given elsewhere on the EIS wiki.
!Exercises
For these exercises you will need to refer to the [EIS object methods page|EISmethods].
#Create and plot an IDL map for the Fe XII 195.12 line by taking the moments of the line.
#Now use the getvar() method to extract the 195.12 wavelength window. Sum the 3D window over the wavelength direction (use the IDL total() routine), and plot the resulting image. How does it compare to the map image plotted above? See the object methods page for why it is different.
#Using the following commands, can you work out the direction that EIS rasters? (east-west, or west-east)
{{{
IDL> ti=data->getti_1()
IDL> sec=data->sec_from_obs_start(ti)
IDL> xpos=data->getxpos()
}}}