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SYGP: Symposium Gemeinsame Probleme in Fusions- und astrophysikalischen Plasmen
SYGP 2: Posters
SYGP 2.3: Poster
Montag, 12. März 2012, 16:00–16:30, Poster.V
Experimental investigations on expanding magnetic flux ropes — •Philipp Kempkes1, Felix Mackel2, Sascha Ridder2, Thomas Tacke2, and Henning Soltwisch2 — 1MPI for Plasma Physics, 17491 Greifswald — 2Ruhr-Universität Bochum, 44780 Bochum
Twisted magnetic flux ropes show complex dynamic behaviour on different temporal and spacial scales. A prominent example for these confiugurations are arch-shaped solar prominences which can be stable for long periods before becoming eruptive. The FlareLab experiment is designed to investigate the evolution of expanding arch-shaped magnetic flux ropes. Recently, the experiment has been equipped with a new plasma source which provides more flexibility in the magnetic field configuration. It is aimed at following the model considerations proposed by Titov and Démoulin [1] as a descriptive model for a certain class of solar phenomena. First results obtained with the improved plasma source are presented in this contribution. Differences of the magnetic topology as compared to the previous plasma source design are shown and the corresponding influence on the discharge evolution is investigated.
[1] V.S. Titov and P. Démoulin, Astron. Astrophys. 351, 707 (1999)