Determination of 3D Trajectories of Knots in Solar Prominences Using MSDP Data

Details Determination of 3D Trajectories of Knots in Solar Prominences Using MSDP Data Determination of 3D Trajectories of Knots in Solar Prominences Using MSDP Data

2010-10-15

arxiv.org/abs/1010.3152v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

14 pages, 9 figures, accepted for publication in Solar Physics

Scientific paper

In this paper we present a new method of restoration of the true thee-dimensional trajectories of the prominence knots based on ground-based observations taken with a single telescope, which is equipped with a Multi-Channel Subtractive Double Pass imaging spectrograph. Our method allows to evaluate true three-dimensional trajectories of the prominence knots without any assumptions concerning the shape of the trajectories or dynamics of the motion. The reconstructed trajectories of several knots observed in three prominences are presented.

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