3D evolution of an eruptive prominence of 15 May 2000 and the associated active phenomena

Details 3D evolution of an eruptive prominence of 15 May 2000 and the associated active phenomena 3D evolution of an eruptive prominence of 15 May 2000 and the associated active phenomena

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.535..507r&link_type=abstract

In: Solar variability as an input to the Earth's environment. International Solar Cycle Studies (ISCS) Symposium, 23 - 28 June 2

Astronomy and Astrophysics

Astronomy

1

Solar Prominences, Coronal Mass Ejections, Solar Flares

Scientific paper

An eruptive prominence associated with solar flare and CME was observed at the eastern part of the solar limb on 15 May 2000 with the Small Coronagraph, Large Coronagraph and the MSDP (spectral imagery) of the Astronomical Institute of the Wroclaw University. A 3D evolution of the prominence was established on the basis of Hα images and spectra. The same prominence was observed also by Karlický and co-authors 2001 with a classical multi-camera spectrograph of the Ondrejov Observatory. The presented report briefly compares the results of the both analyses of the prominences' structure and evolution, obtained on the basis of the classical spectroscopic and MSDP spectra-imagery data.

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