Eruption Characteristics of a Large Filament

Details Eruption Characteristics of a Large Filament Eruption Characteristics of a Large Filament

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agusmsp43a..05b&link_type=abstract

American Geophysical Union, Spring Meeting 2008, abstract #SP43A-05

Astronomy and Astrophysics

Astrophysics

7500 Solar Physics, Astrophysics, And Astronomy, 7507 Chromosphere, 7524 Magnetic Fields, 7531 Prominence Eruptions, 7599 General Or Miscellaneous

Scientific paper

Erupting filaments are often precursors to mass ejections. We present chromospheric observations of a large erupting filament observed on November 7, 2003. Using trajectory tracking algorithms, we follow the dynamics of this eruption over several hours, in an effort to understand the structural reorganization of filaments during an eruption. This analysis provides clues to the magnetic structure of filaments, and a model for the expansion of conical structures containing twisted magnetic fields.

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