Title of article
Magnetic confinement in the solar interior
Author/Authors
Toby S. Wood، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2010
Pages
2
From page
409
To page
410
Abstract
The observed uniform rotation of the Sun’s radiative interior can be explained by the presence of a global-scale interior magnetic field, provided that the field remains confined below the convection zone. In high latitudes, such magnetic confinement is possible by means of persistent downwelling, driven by the convection zone’s turbulent stresses.
Keywords
MHD , Sun: abundances , Sun: interior , Sun: rotation , Sun: magnetic fields
Journal title
Proceedings of the International Astronomical Union
Serial Year
2010
Journal title
Proceedings of the International Astronomical Union
Record number
667795
Link To Document