TL;DR
This study analyzes the latitudinal migration of solar filaments over multiple solar cycles and compares it with sunspot group movements to understand underlying physical processes.
Contribution
It provides a detailed comparison of filament and sunspot latitudinal drifts across cycles, highlighting their physical implications.
Findings
Filaments show latitudinal migration patterns similar to sunspots.
Latitudinal drift varies between hemispheres and cycles.
Physical implications suggest underlying solar magnetic field dynamics.
Abstract
The Carte Synoptique catalogue of solar filaments from March 1919 to December 1989, corresponding to complete cycles 16 to 21 is utilized to show latitudinal migration of filaments at low latitudes (less than 50 deg), and the latitudinal drift of solar filaments in each hemisphere in each cycle of the time interval is compared with the corresponding drift of sunspot groups. The physical implication behind the latitudinal drift of filaments is explored.
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