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

Дата и время публикации : 2010-10-15T13:14:39Z

Авторы публикации и институты :
Maciej Zapior
Pawel Rudawy

Ссылка на журнал-издание: Ссылка на журнал-издание не найдена
Коментарии к cтатье: 14 pages, 9 figures, accepted for publication in Solar Physics
Первичная категория: astro-ph.SR

Все категории : astro-ph.SR

Краткий обзор статьи: 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.

Category: Physics