Abstract
Precise measurements of heliographic position of solar filaments were used for determination of the proper motion of solar filaments on the time-scale of days. The filaments have a tendency to make a shaking or waving of the external structure and to make a general movement of whole filament body, coinciding with the transport of the magnetic flux in the photosphere. The velocity scatter of individual measured points is about one order higher than the accuracy of measurements.
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Ambrož, P., Schroll, A. Large-scale motion of solar filaments. J Astrophys Astron 21, 205–208 (2000). https://doi.org/10.1007/BF02702392
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DOI: https://doi.org/10.1007/BF02702392