Magnetohydrodynamic Stability of a High-Speed Ejective Cylinder in Solar Atmosphere

Details Magnetohydrodynamic Stability of a High-Speed Ejective Cylinder in Solar Atmosphere Magnetohydrodynamic Stability of a High-Speed Ejective Cylinder in Solar Atmosphere

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983acasn..24..208c&link_type=abstract

Acta Astronomica Sinica, Vol.24, NO.3, P.208, 1983

Astronomy and Astrophysics

Astronomy

Scientific paper

Using the dispersion equation of the stability of a plasma cylinder which was deduced in the case of existing internal flow, the dispersion curves of the growing mode have been calculated for the internal velocity of 160 km/s (surge type) and 600 km/s (spray type) respectively. Physical explanations were made for several special high-speed ejective phenomena.

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