Inversion of Physical Parameters in Solar Coronal Magnetic Structures

Bibcode
2012ASPC..456..121A
Arregui, I..; Ballester, J.; Goossens, M.; Oliver, R.; Asensio-Ramos, A.
Referencia bibliográfica

The Fifth Hinode Science Meeting. ASP Conference Series, Vol. 456, Proceedings of a conference held 10-14 October 2011 at Royal Sonesta Hotel, Cambridge, Massachusetts. Edited by Leon Golub, Ineke De Moortel and Toshifumi Shimizu. San Francisco: Astronomical Society of the Pacific, 2012., p.121

Advertised on:
5
2012
Número de autores
5
Número de autores del IAC
1
Número de citas
1
Número de citas referidas
1
Descripción
Magnetohydrodynamic seismology aims to determine difficult to measure physical parameters in the solar corona by a combination of observed and theoretical properties of waves and oscillations. We describe relevant examples of the application of seismology techniques to transversely oscillating coronal loops and prominence fine structures. We also show how the use of statistical techniques, based on Bayesian inference, can be of high value in the determination of physical parameters in these structures, by consistently taking into account the information from observations.
Tipo
Sin árbitro

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