Hostname: page-component-78c5997874-mlc7c Total loading time: 0 Render date: 2024-11-03T08:42:10.536Z Has data issue: false hasContentIssue false
  • English
  • Français

Magnetic fields in the Solar Nebula and the angular momentum transfer

Published online by Cambridge University Press:  03 August 2017

M. Kiguchi ,
S. Narita ,
T. Terasawa  and
C. Hayashi
M. Kiguchi
Affiliation:
Research Institute for Science and Technology, Kinki University, Osaka, 577, Japan
S. Narita
Affiliation:
Department of Electronics, Doshisha University, Kyoto, 602, Japan
T. Terasawa
Affiliation:
Department of Geophysics, Kyoto University, Kyoto, 606, Japan
C. Hayashi
Affiliation:
Kyoto University, Kyoto, 606, Japan

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Type
Poster Sessions
Information
Symposium - International Astronomical Union , Volume 147: Fragmentation of Molecular Clouds and Star Formation , 1991 , pp. 441 - 442
Copyright
Copyright © Kluwer 1991 

References

Hayashi, C., 1981, Prog. Theor. Phys., suppl. 70, 35.Google Scholar
Mouschovias, T.C., Paleologou, E.V., 1979, Ap. J. 230, 204.Google Scholar