Global distribution of filaments during solar cycle No. 20

Details Global distribution of filaments during solar cycle No. 20 Global distribution of filaments during solar cycle No. 20

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...44..225h&link_type=abstract

Solar Physics, vol. 44, Sept. 1975, p. 225-230.

Physics

25

Photosphere, Solar Activity Effects, Solar Cycles, Solar Magnetic Field, Magnetometers, Polar Regions, Recording Instruments, Topology

Scientific paper

By tracing the positions of filaments on the solar disk for a series of consecutive Carrington rotations, one can make a compact representation of the changes in general topology of photospheric magnetic fields during the course of a solar cycle. Examples are shown for the time period 1964-1974, which may provide some insight into the long-term relationship of the mid-latitude diagonal filaments and the high latitude polar crown.

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