Mechanism of mass outflow from the sun in transient phenomena

Details Mechanism of mass outflow from the sun in transient phenomena Mechanism of mass outflow from the sun in transient phenomena

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976azh....53.1264u&link_type=abstract

Astronomicheskii Zhurnal, vol. 53, Nov.-Dec. 1976, p. 1264-1269. In Russian.

Astronomy and Astrophysics

Astronomy

Chromosphere, Solar Corona, Solar Prominences, Astronomical Models, Magnetohydrodynamic Waves, Shock Wave Interaction, Solar Atmosphere, Solar Magnetic Field

Scientific paper

A mechanism is proposed that can explain the observed high-velocity mass ejections from the corona referred to as transients. Transients, eruptive prominences, and chromospheric spray-type surges are considered to result from the successive passage of strong shock waves across the extremely inhomogeneous discontinuties in the solar atmosphere at the chromosphere-corona and prominence-corona boundaries. Calculations are performed which can be used to interpret the observed characteristics of solar transients.

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