Formation of a multi-thread prominence

Details Formation of a multi-thread prominence Formation of a multi-thread prominence

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21640512l&link_type=abstract

American Astronomical Society, AAS Meeting #216, #405.12; Bulletin of the American Astronomical Society, Vol. 41, p.891

Astronomy and Astrophysics

Astronomy

Scientific paper

Solar prominences are composed of many threads of cool and dense plasma suspended in the million-degree solar corona. We have constructed a 3D time-dependent model of a prominence from 1D independent simulations of many flux tubes. The 3D magnetic field is taken from an adaptive MHD simulation of a sheared double-arcade filament channel. We will show the evolving properties of our model prominence and compare the results with data from telescopes onboard the SOHO, STEREO, and Hinode satellites.

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