Exact 2D MHD modelling of coronal loops observed with TRACE and CDS including comprssible flow and heating.

Details Exact 2D MHD modelling of coronal loops observed with TRACE and CDS including comprssible flow and heating. Exact 2D MHD modelling of coronal loops observed with TRACE and CDS including comprssible flow and heating.

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506..713p&link_type=abstract

In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze

Physics

Solar Coronal Loops: Magnetohydrodynamics, Heating

Scientific paper

We present exact models of coronal loops including heating, which can be compared quantitatively to observational data. The systematic nonlinear separation of variables method used to calculate the equilibria has already been developed in spherical geometry and in Cartesian geometry generalising many known solutions. Using a particularly versatile solution class in Cartesian geometry with a large parameter space we are able to calculate models whose loop length, loop shape, plasma density, temperature and velocity profiles are fitted to loops observed with TRACE and with SoHO CDS, while consistent heating profiles are also given.

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