Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..90..391h&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 90, no. 2, Feb. 1983, p. 391-403.
Astronomy and Astrophysics
Astrophysics
6
Magnetic Field Configurations, Polarity, Solar Magnetic Field, Spherical Coordinates, Equatorial Regions, Magnetic Dipoles, Magnetostatics, Plasma Density, Polar Regions, Stellar Magnetic Fields
Scientific paper
The non-axisymmetric and nonlinear solutions of the magnetostatic equations are given in three-dimensional space of spherical coordinates. These solutions are applied to the large-scale solar magnetic field. Their basic features are similar to a dipole field near the polar regions and the polarity reverses near the equator. These features agree with observations for the large-scale solar magnetic field. The solutions can also be applied to investigate the connection between the structure of the magnetic field and the density distribution of the corona. It is shown that the tops of the closed magnetic field associate with density enhancements. Similar results may apply to the large-scale configuration of the stellar field.
No associations
LandOfFree
The non-axisymmetrical configuration of a large-scale solar and stellar magnetic field does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The non-axisymmetrical configuration of a large-scale solar and stellar magnetic field, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The non-axisymmetrical configuration of a large-scale solar and stellar magnetic field will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1305561