Large-amplitude oscillations in solar prominences derived from high-resolution simulations | Valeriia Liakh
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19.05.2021
Co-author
Affiliation
Instituto de Astrofísica de Canarias (IAC)
Main category
Natural Sciences (Astrophysics and Astrononmy)
Caption
We report 2D MHD simulations of the large-amplitude oscillations (LAOs) in the solar prominences performed with MHD code Mancha. We aim to study the properties of LAOs using high-resolution simulations in a simple 2D magnetic configuration that contains a dipped part. We loaded the dense prominence plasma in the dips region. In order to excite oscillations, we used a perturbation directed along the magnetic field. For the same numerical model, the four spatial resolutions were considered: 240, 120, 60, and 30 km. The longitudinal LAOs (LALOs) are strongly damped even in the high-resolution simulation in the region of the weaker and more curved magnetic field (at the center and bottom of the prominence). At the prominence top, the oscillations have relatively longer damping times. Furthermo
Further information
Further reading
Link to the European Solar Physics Online Seminars (ESPOS) webpage: https://espos.stream/2021/03/25/Liakh/
Language
English
DOI
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