Publication Date:
2019-06-27
Description:
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.
Keywords:
SPACE RADIATION
Type:
NASA-CR-139501
,
SU-IPR-570
Format:
application/pdf