This page (revision-23) was last changed on 28-Aug-2023 22:31 by Peter Young

This page was created on 26-Jul-2007 22:00 by Mike Smith

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
23 28-Aug-2023 22:31 4 KB Peter Young to previous
22 11-Jul-2023 17:09 4 KB akadojewu to previous | to last
21 03-Nov-2016 18:34 6 KB utijeyer to previous | to last

Page References

Incoming links Outgoing links
EisDiscussion
EisDiscussion

Version management

Difference between version and

At line 2 removed one line
All related materials go here, thanks.
At line 4 removed one line
At line 5 added one line
!A Comment on Using Fe XII 195 for Studying Nonthermal Widths and Doppler Shifts
At line 7 added one line
Fe XII 195 is a core line and is present in almost every EIS study. It has been noted, however, that there is a subtle contribution of Fe XII 195.18 to the wing of the observed line profile. This component is density senitive and can make an important contribution to the line in active regions. The intensity of this component is generally very small (<15% of the total), it does, however, alter the calculation of the line width and centroid. The following images illustrate the
At line 10 removed one line
----
At line 12 removed one line
I think this isn't for anything
At line 14 removed 8 lines
--[David R Williams|http://null], 18-Mar-2009
_________________________________________________
I thought there was to be an area for presenting a short description of various science results
Ken Dere (3/23/09)
This page (revision-23) was last changed on 28-Aug-2023 22:31 by Peter YoungTop