Current instability and generation of Alfven waves in coronal loops

Details Current instability and generation of Alfven waves in coronal loops Current instability and generation of Alfven waves in coronal loops

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992kfnt....8...20m&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 8, Jan.-Feb. 1992, p. 20-23. In Russian.

Physics

1

Coronal Loops, Current Density, Magnetic Field Reconnection, Magnetohydrodynamic Stability, Magnetohydrodynamic Waves, Photosphere, Solar Atmosphere, Solar Flares

Scientific paper

Current instability of MHD waves in coronal loops is analyzed. It is
shown that this instability may develop effectively only at the top of
the loop in the corona, where plasma density is sufficiently low. The
development of disturbances can promote the reconnection of magnetic
fields and thus stimulate flare development.

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