Theoretical analysis of iron X-ray spectra observed in solar active region.
Abstract
The theoretical analysis of X-ray spectra observed by the Flat Crystal Spectrometer of the Solar Maximum Mission in the 13 Å - 19 Å wavelength range is presented. The emission lines correspond to Fe ions (Fe XVI, Fe XVII, Fe XVIII) and some O-ions (O VII, O VIII). The fitting of a synthetic spectrum to the observed one shows that it is difficult to represent the emissive region with one temperature model.
- Publication:
-
5. Internationale Konferenz über die Physik hochgeladener Ionen
- Pub Date:
- 1991
- Bibcode:
- 1991phgi.conf..159C