The Structure of the Chromosphere Properties Pertaining to Element Fractionation

Details The Structure of the Chromosphere Properties Pertaining to Element Fractionation The Structure of the Chromosphere Properties Pertaining to Element Fractionation

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ssrv...85..187j&link_type=abstract

Space Science Reviews, Volume 85, Issue 1-2, pp. 187-202

Physics

18

Sun:Chromosphere, Abundance Patterns

Scientific paper

We review the structure and dynamics of the solar chromosphere with emphasis on the quiet Sun and properties that are relevant to element fractionation mechanisms. Attention is given to the chromospheric magnetic field, its connections to the photosphere, and to the dynamical evolution of the chromosphere. While some profound advances have been made in the “unmagnetized” chromosphere, our knowledge of the magnetically controlled chromosphere, more relevant for the discussion of element fractionation, is limited. Given the dynamic nature of the chromosphere and the poorly understood magnetic linkage to the corona, it is unlikely that we will soon know the detailed processes leading to FIP fractionation.

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