Physics
Scientific paper
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.
Karlicky Marian
Šimberová Stanislava
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