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    In:  CASI
    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
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