Implications of Coronal Abundance Variations

Details Implications of Coronal Abundance Variations Implications of Coronal Abundance Variations

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994kofu.symp..305s&link_type=abstract

In: Proceedings of Kofu Symposium, Kofu, Japan, Sept. 6-10, 1993, p.305-308.

Computer Science

1

Scientific paper

High resolution soft X-ray spectra acquired by the Flat Crystal Spectrometer on Solar Maximum Mission have yielded exciting new information on the composition of the dynamic corona above solar active regions. In the brightest parts of these regions, the relative abundances of O, Ne, Mg, and Fe are found to vary from photospheric composition values to (and beyond) the typical ``coronal'' values found for solar energetic particles. This abundance variability complicates data interpretation but may ultimately offer new clues to the processes which supply and heat the corona.

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