Reconnection in adjoining coronal helmet streamers

Details Reconnection in adjoining coronal helmet streamers Reconnection in adjoining coronal helmet streamers

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..19.1887d&link_type=abstract

Advances in Space Research, vol. 19, p. 1887

Computer Science

3

Solar Magnetic Field, Magnetic Field Reconnection, Solar Corona, Current Sheets, Magnetohydrodynamic Stability, Magnetohydrodynamic Flow, Magnetohydrodynamic Waves, Wakes, Propagation Modes

Scientific paper

Both wake flows and multiple current sheets are known to be independently unstable; it is here proposed that instabilities in the combined system might account for the complex flows and structures observed in adjoining streamers. It is shown that while the structure of the modes is significantly changed by the Alfvenic and sub-Alfvenic wake flow, their growth rates are not changed.

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