Dynamics of the solar magnetic field. V - Velocities associated with changing magnetic fields

Mathematics – Logic

Scientific paper

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Magnetic Signatures, Solar Flares, Solar Magnetic Field, Velocity Distribution, Flow Distribution, Magnetic Induction, Solar Atmosphere

Scientific paper

Methods of determining horizontal velocities from the magnetic induction equation on the basis of a time series of magnetogram observations are discussed. For the flare of 1972 August 7, it is shown that a previously developed method of predicting positions of likely flare activity provides reasonable agreement with observations. Limitations to this type of solution of the magnetic induction equation are pointed out, and unambiguous solutions, corresponding to phenomenological determinations of velocity patterns under various physical circumstances, are presented for simple magnetic configurations. Implications for the analysis of changes in a series of magnetogram observations are discussed.

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