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Transverse Oscillations in Coronal Loops

Bibcode
2007AIPC..934...54A
DOI
10.1063/1.2790358
Arregui, I.; Luna, M.; Oliver, R.; Terradas, J.; Ballester, J. L.
Referencia bibliográfica

FLOWS, BOUNDARIES, INTERACTIONS: Flows, Boundaries, and Interaction Workshop. AIP Conference Proceedings, Volume 934, pp. 54-63 (2007).

Fecha de publicación:
9
2007
Número de autores
5
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
During last years, direct evidence about oscillations in different coronal structures has been obtained thanks to the detailed observations made by SoHO and TRACE. With the help of magnetohydrodynamic (MHD) wave theory, we can explain these observations as due to the excitation and propagation of MHD waves in the solar corona. In spite that there are many solar coronal structures in which oscillations have been detected (prominences, loops, plumes, coronal holes, etc.), in the following we will concentrate on transverse oscillations of coronal loops, reviewing some theoretical models developed to understand these oscillations in terms of MHD waves.
Tipo
Sin árbitro
Bucles coronales

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