Steady models for th hard X-ray loops in the solar corona

Details Steady models for th hard X-ray loops in the solar corona Steady models for th hard X-ray loops in the solar corona

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...91..311t&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 91, April 1984, p. 311-324.

Physics

12

Coronal Loops, Solar Corona, Solar Flares, Solar X-Rays, Conductive Heat Transfer, Confinement, Dense Plasmas, High Temperature Plasmas

Scientific paper

Two stationary models are proposed for the hot thermal loops observed in 14-40 keV X-rays over nearly the entire phase of solar flares, together with the similar, but softer 5-10 keV X-ray loop. In the first model, the high density loop possesses a sufficiently high plasma density to lose the conduction flux from the summit, due to hot loop radiation. The foot points may accordingly not be bright in H-alpha. In the second model, loops of either higher temperature or lower density than those of the first model are seen as having a negligibly small loop radiation loss by comparison with the conduction flux; the heat flux along the loop is accordingly almost entirely converted into a chromospheric flow.

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