Non-local heat transport in static solar coronal loops

Details Non-local heat transport in static solar coronal loops Non-local heat transport in static solar coronal loops

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991soph..132..279c&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 132, April 1991, p. 279-291.

Physics

4

Coronal Loops, Heat Transfer, Solar Corona, Thermal Conductivity, Scaling Laws, Stellar Models

Scientific paper

The limits of applicability of the Spitzer-Harm thermal conductivity in solar coronal loops is investigated, and it is shown that the ratio of electron mean-free path to temperature scale height in large-scale structures can approach the limits of the Spitzer-Harm theory. A nonlocal formulation of heat transport is used to compute a grid of loop models: the effects of nonlocal transport on the distribution of differential emission measure are particularly important in the coronal part of loops longer than the pressure scale height.

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