Solar Physics

, Volume 25, Issue 1, pp 5–13

Polar magnetic fields of the Sun: 1960–1971

  • Robert Howard
Article

DOI: 10.1007/BF00155740

Cite this article as:
Howard, R. Sol Phys (1972) 25: 5. doi:10.1007/BF00155740

Abstract

Observations of the magnetic fields in the polar regions of the Sun are presented for the period 1960–1971. At the start of this interval the fields at the two poles were consistently of opposite sign and averaged around 1 G. Early in 1961 the field in the south decreased suddenly and the field in the north decreased in strength slowly over the next few years. By the mid-1960's the fields at both poles were quite weak and irregular. Throughout the period of these observations the fields at both poles often showed a remarkable tendency to vary in unison. About the middle of 1971 the north polar field became significantly positive, first at lower latitudes, then above 70 °. An autocorrelation analysis of the polar fields in the north shows a weak rotation peak, indicating significant ‘features’ in these regions. A comparison of field strengths in the east and west quadrants in the north suggests that even at the extreme polar latitudes the following polarity fields are inclined slightly toward the rotation and the preceding polarity field lines are inclined slightly to trail the rotation.

Copyright information

© D. Reidel Publishing Company 1972

Authors and Affiliations

  • Robert Howard
    • 1
  1. 1.Hale Observatories, Carnegie Institution of Washington, California Institute of TechnologyPasadenaU.S.A.