Plasma Flows in Coronal Loops

Details Plasma Flows in Coronal Loops Plasma Flows in Coronal Loops

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21630004y&link_type=abstract

American Astronomical Society, AAS Meeting #216, #300.04; Bulletin of the American Astronomical Society, Vol. 41, p.815

Astronomy and Astrophysics

Astronomy

Scientific paper

A survey of plasma flows in coronal loops is underway using data from the Hinode/EIS instrument. The principal target is a study of flows in 1 MK (so-called 'warm' loops). Using emission lines formed between logT=5.6 and 6.2 it is possible to study the temperature dependence of the flows, and also the density of the emitting material. The results will be critical to making a definitive statement about whether apparent motions seen in TRACE 171 movies are due to actual mass motion or wave propagation. In addition we will also comment on the relation between the flows in warm loops and those in the newly-discovered active region outflow regions found by Hinode.

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