Analytic Approximate Seismology of Propagating Magnetohydrodynamic Waves in the Solar Corona

Bibcode
2012ApJ...760...98G
DOI
10.1088/0004-637X/760/2/98
Goossens, M.; Soler, R.; Arregui, I.; Terradas, J.
Referencia bibliográfica

The Astrophysical Journal, Volume 760, Issue 2, article id. 98, 8pp, (2012).

Fecha de publicación:
12
2012
Revista
The Astrophysical Journal
Número de autores
4
Número de autores del IAC
1
Número de citas
19
Número de citas referidas
18
Descripción
Observations show that propagating magnetohydrodynamic (MHD) waves are ubiquitous in the solar atmosphere. The technique of MHD seismology uses the wave observations combined with MHD wave theory to indirectly infer physical parameters of the solar atmospheric plasma and magnetic field. Here, we present an analytical seismological inversion scheme for propagating MHD waves. This scheme uses the observational information on wavelengths and damping lengths in a consistent manner, along with observed values of periods or phase velocities, and is based on approximate asymptotic expressions for the theoretical values of wavelengths and damping lengths. The applicability of the inversion scheme is discussed and an example is given.
Proyectos relacionados
Erupción solar
Simulación Numérica de Procesos Astrofísicos

La simulación numérica mediante códigos complejos de ordenador es una herramienta fundamental en la investigación física y en la técnica desde hace décadas. El crecimiento vertiginoso de las capacidades informáticas junto con el avance notable de la matemática numérica ha hecho accesible a los centros de investigación de tamaño medio

Daniel Elías
Nóbrega Siverio
En ejecución
Tipo
Con árbitro
Campos magnéticos
Física Solar (FS)

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