3d trajectories of plasma blobs in solar eruptive and active prominences

Details 3d trajectories of plasma blobs in solar eruptive and active prominences 3d trajectories of plasma blobs in solar eruptive and active prominences

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010nspm.conf..100z&link_type=abstract

Proceedings of the 20th National Solar Physics Meeting, held 31 May - 4 June, 2010 in Papradno, Slovakia, p. 100

Physics

Scientific paper

We present a unique method of reconstruction of the true 3D trajectories of the prominence blobs observed with the Multi-channel Subtractive Double Pass imaging spectrographs. Using data collected with the Wroclaw MSDP spectrograph installed on Large Coronagraph, trajectories of the blobs of numerous active and eruptive prominences were reconstructed, showing their 3D structure and temporal evolution of their magnetic skeletons. As examples of the obtained results we present reconstructed trajectories of several blobs in three prominences. The unique results that we obtained are very useful in analysis of the prominence eruptions and their connections with CMEs.

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