From: Isabelle Ruedi
Date: 2 April 1998


EIT/CDS:
For us, it is of advantage if the EIT Full disk (high resolution) synoptic 
images are recorded during the CDS raster. Or, the closer the better.

MDI:
The CDS sequence lasts approximately two hours, so that we will have one of the 
96 min magnetogram overlapping the CDS sequence anyway.

Here is the actual line list. Since the windows have a width of 36 pixels (only 
for the high telemetry), the wavelength of the window is only given very 
approximately. Note, that this line list does not replace the old one, but
replaces it at time of high CDS telemetry.


CDS Study description:
---------------------

Slit: 2" x 240"
Number of points retained along the slit: 143
Width of spectral boxes: 36 pixels
Raster step width: 2"
Number of step: 120 
Compression: 16 to 12 bits
Exposure time: 60s

   Line    Wavelength  Central pixel

1) MgVII,SiVIII   319  170
2) FeXIV, FeXVI   334  388
3) FeXII,MgVIII   338  445
4) SiX            347  567
5) MgVI,SiIX      349  597 
6) FeXIV          353  662
7) SiX            356  689
8) FeXIII, FeXVI  359  750   
9) MgVII-IX       368  862
10) SiXII         520  65 
11) OIII          525  110
12) NeIV          541  245
13) OIV           554  355
14) CaX           557  387
15) NeV           572  514 
16) HeI           584  610 
17) FeXIX         592  681 
18) OIII          599  740 
19) MgX           624  960
20) OV            629 1000