Solar Rotating Magnetic Dipole.
Abstract
A magnetic dipole rotating around an axis perpendicular to the rotation axis of the sun can account for the characteristics of the surface large-scale solar magnetic fields through the solar cycle. The polarity patterns of the interplanetary magnetic field, predictable from this model, agree with the observed interplanetary magnetic sector structure. (Author)
Document Details
- Document Type
- Technical Report
- Publication Date
- Apr 26, 1974
- Accession Number
- AD0784428
Entities
People
- Ester Antonucci
Organizations
- Stanford University