Formation of a multi-thread prominence

Bibcode
2010AAS...21640512L
Luna Bennasar, Manuel; Karpen, J. T.; DeVore, C. R.
Bibliographical reference

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

Advertised on:
5
2010
Number of authors
3
IAC number of authors
0
Citations
0
Refereed citations
0
Description
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.
Type
Non-refereed

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