On build-up of magnetic energy in the so
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Y. Nakagawa; R. S. Steinolfson; S. T. Wu
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Article
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1976
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Springer
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English
β 477 KB
The dynamic response of the solar atmosphere is examined with the use of self-consistent numerical solutions of the complete set of nonlinear, two-dimensional, hydromagnetic equations. Of particular interest are the magnetic energy build-up and the velocity field established by emerging flux at the