Modeling Coronal Loop Abundances: Effects of Parameter Variations on Observables

Details Modeling Coronal Loop Abundances: Effects of Parameter Variations on Observables Modeling Coronal Loop Abundances: Effects of Parameter Variations on Observables

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000soph..193..131l&link_type=abstract

Solar Physics, v. 193, Issue 1/2, p. 131-137 (2000).

Physics

1

Scientific paper

Coronal abundance variations arise from and affect solar atmospheric processes such as coronal heating and structural dynamics. Lenz (1999) presented initial results of a numerical theoretical study of abundances and ion heating rates in static, steady-state coronal loops. We present here a closer investigation of two fundamental aspects of the physics of coronal abundances, relating modeling parameters to observables: (1) the effect of varying the abundances on the electron temperature and (2) the effect of varying the ion heating rate on abundances.

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