Inference of physical parameters in solar prominence threads

Montes-Solís, M.; Arregui, I.
Referencia bibliográfica

Highlights on Spanish Astrophysics X, Proceedings of the XIII Scientific Meeting of the Spanish Astronomical Society held on July 16-20, 2018, in Salamanca, Spain, ISBN 978-84-09-09331-1. B. Montesinos, A. Asensio Ramos, F. Buitrago, R. Schödel, E. Villaver, S. Pérez-Hoyos, I. Ordóñez-Etxeberria (eds.) p. 514-519

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3
2019
Número de autores
2
Número de autores del IAC
2
Número de citas
0
Número de citas referidas
0
Descripción
We consider magnetohydrodynamics models and observations of transverse oscillations in prominence threads to obtain information on their physical properties such as the magnetic field strength, the plasma density, or the length. We further compare between short and long thread limits in period ratio models and compute the relative plausibility of alternative mechanisms in explaining the observed damping of transverse oscillations. Bayesian techniques are used for both analyses. The results show that the physical parameters of interest can be inferred. Values of period ratio around 1 are more likely in the long thread limit while shorter and larger values are more likely in the short thread limit. The mechanism known as resonant absorption in the Alfvén continuum is the most plausible damping mechanism.