Time distribution of the long-lived filaments in the years 1931-1987

Details Time distribution of the long-lived filaments in the years 1931-1987 Time distribution of the long-lived filaments in the years 1931-1987

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..140..195d&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 140, no. 1, July 1992, p. 195-198.

Physics

Free Convection, Magnetohydrodynamic Stability, Solar Cycles, Solar Flares, Magnetic Flux, Periodic Variations, Solar Activity, Solar Magnetic Field

Scientific paper

The dependence of the number and lifetime distribution of the filaments in the solar cycle phase is analyzed for those filaments that exist for two or more rotations. A long-term variation in the distributions of the filaments is noted and related to the changes in full magnetic flux. The behavior of the filaments is of interest for tracing active-region magnetic fields that can shed light on processes in the solar convection zone.

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