High latitude solar magnetic fields

Details High latitude solar magnetic fields High latitude solar magnetic fields

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..138..419m&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 138, no. 2, April 1992, p. 419-422.

Physics

6

Magnetic Signatures, Solar Activity Effects, Solar Magnetic Field, Limb Darkening, Pixels, Solar Limb, Solar Physics

Scientific paper

Kitt Peak magnetograms are used to measure polar magnetic fields. The polar mean absolute field increases at the same time as the polar mean field decreases. That is, the polar mean absolute field varies in phase with solar activity, in contrast to the out of phase variation of the mean polar field. It is found that the polar fields have a large bipolar component even at solar minimum, with a magnitude equal to that found at low latitudes outside the active latitude bands.

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