Effects of Large-Scale Flows on Coronal Abundances: Multispecies Models and TRACE Observations

Details Effects of Large-Scale Flows on Coronal Abundances: Multispecies Models and TRACE Observations Effects of Large-Scale Flows on Coronal Abundances: Multispecies Models and TRACE Observations

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003spd....34.1703l&link_type=abstract

American Astronomical Society, SPD meeting #34, #17.03; Bulletin of the American Astronomical Society, Vol. 35, p.837

Astronomy and Astrophysics

Astronomy

Scientific paper

Understanding coronal abundances is crucial for interpreting coronal observations and for understanding coronal physical processes and heating. Bulk flows and gravity, both unmistakably present in the corona, significantly affect abundances. We present multispecies simulations of long-lived coronal structures and compare model results with TRACE observations, focusing on abundance variations and flows.

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