Determination of 3D Trajectories of Knots in Solar Prominences Using MSDP DataReport as inadecuate




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Solar Physics

, Volume 267, Issue 1, pp 95–105

First Online: 23 October 2010Received: 30 June 2010Accepted: 19 September 2010

Abstract

In this paper we present a new method of restoration of the true three-dimensional 3D trajectories of prominence knots using ground-based observations taken with a single telescope that is equipped with a Multi-Channel Subtractive Double Pass imaging spectrograph. Our method allows us to evaluate the true 3D trajectories of the prominence knots without any assumptions concerning the shape of the trajectories or the dynamics of the motion. The reconstructed trajectories of several knots observed in three prominences are presented.

KeywordsInstrumentation and data management Prominences, dynamics Prominences, formation and evolution Electronic Supplementary MaterialThe online version of this article doi:10.1007-s11207-010-9643-z contains supplementary material, which is available to authorized users.

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Author: Maciej Zapiór - Paweł Rudawy

Source: https://link.springer.com/



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