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Magnetic fields in the Solar Nebula and the angular momentum transfer
Published online by Cambridge University Press: 03 August 2017
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We are now carrying out the project to investigate how the primodial solar disk is formed and evolves. One of the central problems of this project is to study the angular momentum transfer in the nebula caused by the magnetic braking or the turbulent mixing in the boundary layer between the surface of the disk and its high temperature corona envelope.
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