Very low intensity in coronal holes
A number of surrounding weaker lines
Possible multilayers: Si / B4C
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Introduction
Multilayer issues
Line Constraints
Wavelength Options
Dual Lines:
Si XI - He II
Ne VII - Ca IX
Si XI - He I
O IV - Mg X
Mg X - O V
O III - Mg IX
Single Lines:
C VI
Fe IX
Fe X
Fe XIII
Mg IX
Si XII
