Large-scale patterns of prominences in the global solar cycles during 1880-1995Large-scale patterns of prominences in the global solar cycles during 1880-1995
Faculty of Sciences. Physics
Department of Physics
San Francisco, Calif. :Astronomical Soc Pacific, 1998[*]1998
IAU Colloquium 167 on New Perspectives on Solar Prominences, April 28-May 03, 1997, CTR Paul Langevin, Aussois, France
University of Antwerp
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 H-alpha charts (1915-1990) are given.