SpS1-Digging in the solar COmosphere with NAC

Details SpS1-Digging in the solar COmosphere with NAC SpS1-Digging in the solar COmosphere with NAC

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010hia....15..547a&link_type=abstract

Highlights of Astronomy, Volume 15, p. 547-547

Astronomy and Astrophysics

Astronomy

Scientific paper

The solar “COmosphere” is an enigmatic region of cold gas (temperatures as low as ~3500 K) coexisting in the low chromosphere with plasma much hotter (~7000 K). This zone probably consists of patchy clouds of cool gas, seen readily in off-limb emissions of CO 4667 nm lines, threaded by hot gas entrained in long-lived magnetic filaments as well as transient shock fronts. The COmosphere was not anticipated in classical 1D models of the solar outer atmosphere, but is quite at home in the contemporary 3D highly dynamic view, which one might call the Magnetic Complexity Zone.

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