Large-scale motion of solar filaments

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, c...

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Published in:Journal of astrophysics and astronomy 2000-09, Vol.21 (3-4), p.205-208
Main Authors: Ambro, Pavel, Schroll, Alfred
Format: Article
Language:English
Subjects:
Astronomy
Filaments
Magnetic flux
Movement
Photosphere
Scatter
Shaking
Solar physics
Transport
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description 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.
doi_str_mv 10.1007/BF02702392
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subjects Astronomy
Filaments
Magnetic flux
Movement
Photosphere
Scatter
Shaking
Solar physics
Transport
title Large-scale motion of solar filaments
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