Testing Nonuniform Heating RTV-Type Models of Coronal Loops with 3D Differential Emission Measure Tomography

Details Testing Nonuniform Heating RTV-Type Models of Coronal Loops with 3D Differential Emission Measure Tomography Testing Nonuniform Heating RTV-Type Models of Coronal Loops with 3D Differential Emission Measure Tomography

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsh31c1804h&link_type=abstract

American Geophysical Union, Fall Meeting 2010, abstract #SH31C-1804

Astronomy and Astrophysics

Astrophysics

[7509] Solar Physics, Astrophysics, And Astronomy / Corona

Scientific paper

In non-uniform RTV-type loop models, the heating rate is at its maximum at the loop footpoints and decreases exponentially according to the heating scale height h. Here we use a potential field source surface model to generate the loop structures. Then we trace the temperature from 3D Differential Emission Measure Tomography (DEMT) along the loop to get the temperature profile. We will compare this temperature profile with that given by RTV-type models. This is repeated for hundreds of loops and statistical descriptions of the results are given.

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