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Large-Scale Patterns of Prominences in the Global Solar Cycles During 1880–1995

Published online by Cambridge University Press:  12 April 2016

Dirk K. Callebaut ,
Valentine I. Makarov  and
Ksenia S. Tavastsherna
Dirk K. Callebaut
Affiliation:
Physics Dept. UIA, University of Antwerp, B-2610 Antwerp, Belgium
Valentine I. Makarov
Affiliation:
Pulkovo Astronomical Observatory, 196140, St. Petersburg, Russia
Ksenia S. Tavastsherna
Affiliation:
Pulkovo Astronomical Observatory, 196140, St. Petersburg, Russia

Abstract

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The zonal distribution of prominences, their poleward migration from the sunspot zone to the poles, the polar magnetic field reversals and a correlation of the mean latitude of filament bands at minimum activity with the maximum of Wolf number in the next cycle are briefly discussed for the period 1880–1995. The need for research on the longterm latitude distribution of the prominences is emphasized. New results concerning long-term variations of the torsional oscillations of the Sun and quasi-periodic oscillations of the latitude zonal boundaries from an analysis of Hα charts (1915–1990) are given.

Type
Global Patterns
Information
International Astronomical Union Colloquium , Volume 167: New Perspectives on Solar Prominences , 1998 , pp. 442 - 445
Copyright
Copyright © Astronomical Society of the Pacific 1998

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