Formation of a multi-thread prominence

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

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

Fecha de publicación:
5
2010
Número de autores
3
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
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.
Tipo
Sin árbitro

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