Spectroscopic Hinode Observables from Turbulent Heating and Cooling of Coronal Loops

Details Spectroscopic Hinode Observables from Turbulent Heating and Cooling of Coronal Loops Spectroscopic Hinode Observables from Turbulent Heating and Cooling of Coronal Loops

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..397...83b&link_type=abstract

First Results From Hinode ASP Conference Series, Vol. 397, Proceedings of the conference held 20-24 August, 2007, at Trinity Col

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We present a model of coronal loop turbulence allowing the fast computation of heating in a loop at high Reynolds numbers. We also consider the coupling of both heating and cooling processes in loops, including for the first time a feedback of the cooling on the heating: the heating computed by the shell-models used as an input of a hydrodynamic model of a loop with thermal conduction and a self-consistent treatment of radiation. We forward-model spectroscopic variables that can be compared to Hinode observations.

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