Elemental abundances in the upper solar atmosphere

Details Elemental abundances in the upper solar atmosphere Elemental abundances in the upper solar atmosphere

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phst...46..202f&link_type=abstract

Physica Scripta (ISSN 0031-8949), vol. 46, no. 3, Sept. 1992, p. 202-220.

Physics

12

Abundance, Solar Atmosphere, Spectroscopic Analysis, Argon, Energetic Particles, Helium, Neon, Potassium, Solar Corpuscular Radiation, Solar Flares, Solar Wind

Scientific paper

A previous reassessment of spectroscopic abundance measurements from high temperature solar plasmas showed that, on the average, the solar upper atmosphere possesses a composition that is similar in nature to the composition of the solar wind and solar energetic particles. In recent years, an examination of spectra of the upper solar atmosphere has confirmed these results and proceeded to demonstrate that elemental substances change from region to region by as much as an order of magnitude. An account of these changes, a description of the regions in which they occur, and a possible elemental enrichment model are presented.

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