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

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...

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Published in:arXiv.org 2010-10
Main Authors: Zapior, Maciej, Rudawy, Pawel
Format: Article
Language:English
Subjects:
Ground-based observation
Knots
Prominences
Restoration
Solar prominences
Trajectory analysis
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description 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.
doi_str_mv 10.48550/arxiv.1010.3152
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subjects Ground-based observation
Knots
Prominences
Restoration
Solar prominences
Trajectory analysis
title Determination of 3D Trajectories of Knots in Solar Prominences Using MSDP Data
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