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[en] Solution of the nonlinear MHD problem of plasma flow in an increasing dipolar magnetic field is obtained in the approximation of a strong field. The distributions of plasma velocity, displacement, and density are calculated. The situation when the magnetic dipole is 'increased' by rapid process of magnetic reconnection or current sheet rupture is illustrated. Possible applications are discussed in connection with plasma ejections from chromosphere in corona. (Auth.)
Source
Dryer, M. (National Oceanic and Atmospheric Administration, Boulder, CO (USA). Space Environment Lab.); Tandberg-Hanssen, E. (National Aeronautics and Space Administration, Huntsville, AL (USA). George C. Marshall Space Flight Center) (eds.); International Council of Scientific Unions. Special Committee on Solar-Terrestrial Physics; Committee on Space Research. (COSPAR), 75-Paris (France); 577 p; ISBN 90-277-1163-1; 
; 1980; p. 487-489; D. Reidel; Dordrecht, Netherlands; International Astronomical Union symposium no. 91 on solar and interplanetary dynamics; Cambridge, MA, USA; 27 - 31 Aug 1979
; 1980; p. 487-489; D. Reidel; Dordrecht, Netherlands; International Astronomical Union symposium no. 91 on solar and interplanetary dynamics; Cambridge, MA, USA; 27 - 31 Aug 1979