This page (revision-83) was last changed on 02-Feb-2017 13:19 by David R Williams

This page was created on 27-Jan-2009 03:17 by David R Williams

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83 02-Feb-2017 13:19 43 KB David R Williams to previous
82 19-Mar-2009 13:50 41 KB David R Williams to previous | to last
81 18-Mar-2009 21:12 40 KB David R Williams to previous | to last

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At line 529 changed one line
Fe VII: normally see that 195 towers above the rest of the spectrum. The Fe VII data most commonly used are normally in the optical, but now working on the EUV lines.
** Fe VII: normally see that 195 towers above the rest of the spectrum. The Fe VII data most commonly used are normally in the optical, but now working on the EUV lines.
At line 532 added 2 lines
# 11 new line IDs made from EIS spectra (mainly in the LW band)
# 16 new or revised energy levels
At line 535 added 2 lines
*** Diagnostics
Unfortunately no density sensitivity below log ne = 9.0
At line 538 added 13 lines
If you want to put Fe VII in your study, 196.22 is probably the best, and then 195.39 is a factor of two even stronger. Unfortunately, there are a lot of data which have problems and can be out by a factor of two between theory and observations.
Pretty fantastic that you can see 11 consecutive Fe ionisation stages from VII through XVII.
GAD: there's an Fe XXI and XXII line as well as Fe XXIII and XXIV
Also found there are Cr lines, too. Large EM between 5.5 and 5.8 enhances lines in this temperature range. have ID'd Cr VII and Cr VIII
** EIS is very important for doing basic spectroscopy
*** testing atomic data
*** making new identifications
*** benefits existing and upcoming missions' science
This page (revision-83) was last changed on 02-Feb-2017 13:19 by David R WilliamsTop