Modeling of dynamic evolution of roconal loops

Details Modeling of dynamic evolution of roconal loops Modeling of dynamic evolution of roconal loops

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ssrv...70..171s&link_type=abstract

Space Science Reviews, Volume 70, Issue 1-2, pp. 171-174

Computer Science

1

Sun: Corona, Sun: Activity

Scientific paper

Parameters of expanding magnetic loops and arches and of mass flows generated by them in the corona have been computed in a 1D two-fluid approximation. Two possible trigger mechanisms of the coronal transients have been considered: (i) sudden increase of the background magnetic field strength, and (ii) heating and compression plasma inside these magnetic structures. We discuss the formation of shock waves and their dependence on dynamics and geometry of the magnetic structures.

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