EIS spectral ranges and observed emission lines

The wavebands available cover 170-210A and 250-290A. However within the short wavelength
band the reflectivity of the multilayers restrict the performance below 180A and above 204A.

Have a look at the effective areas. To give you an idea of what spectral lines will be observed
in the short (170-210 A) and long wavelength bands (250-290 A) a list of the strongest lines
seen when observing the The Quiet Sun, An Active Region and a Flare are given.

Just click on the region you're interested in. The tables show the strongest lines in each case.

Last Revised: Monday, 24-Jul-2006

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