Emission Lines

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RHESSI observes X-rays down to 3 keV which includes a number of emission lines. They consist mostly of highly ionized Fe lines. There are no lines above about 10 keV.

Lines in RHESSI Spectra
Chianti rhessi 3to30keV.png
Figure 1 from Phillips 2008
Chianti rhessi 6to7keV.png
Chianti rhessi 7to10keV.png

References

Retrieved from "https://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/Emission_Lines"
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