Magnetic rope in the March 20, 2000 prominence eruption

Details Magnetic rope in the March 20, 2000 prominence eruption Magnetic rope in the March 20, 2000 prominence eruption

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.477..127k&link_type=abstract

In: Proceedings of the Second Solar Cycle and Space Weather Euroconference, 24 - 29 September 2001, Vico Equense, Italy. Editor:

Physics

Prominence Eruption, Magnetic Flux Rope

Scientific paper

An evolution of the March 20, 2000 prominence eruption observed in the Hα and 195 Å EIT was analyzed using the image processing technique. The helical structure of the eruptive prominence (magnetic rope) with a hot core was recognized and the electric current of 3.7×1010 Å inside this rope was estimated. The hot core observation agrees with our recent spectroscopic observations. It is interesting that the pre-eruptive filament was located above the X-type photospheric magnetic field. During the eruption the magnetic field changes around this X-type configuration have been found.

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