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NASA NTRS ยท 19720046891

Magnetic energy flow in the solar wind.

Abstract

Discussion of the effect of rotation (tangential flow) of the solar wind on the conclusions of Whang (1971) suggesting an increase in the solar wind velocity due to the conversion of magnetic energy to kinetic energy. It is shown that the effect of the rotation of the sun on the magnetic energy flow results in most of the magnetic energy being transported by magnetic shear stress near the sun.

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BibTeXRIS

Modisette, J. L.. 1972-05-15. Magnetic energy flow in the solar wind.. https://ntrs.nasa.gov/citations/19720046891

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