The relation between the twisting motion of a quiescent filament and the magnetic field.

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

The twisting motion of a quiescent filament in AR5572 was observed on 8 July 1989. Based on the time sequence of magnetograms, Hβ filtergrams and Hβ Dopplergrams obtained at Huairou Solar Observing Station of Beijing Astronomical Observatory, the twisting motion of the filament is identified to be related to three cancelling magnetic features in the filament channel.

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