SciELO - Scientific Electronic Library Online

 
vol.42 número1CCD Photometry of the Globular Cluster M15: RR Lyrae Fourier Decomposition and Physical ParametersMorpho-Kinematic Modeling of Gaseous Nebulae with Shape índice de autoresíndice de materiabúsqueda de artículos
Home Pagelista alfabética de revistas  

Servicios Personalizados

Revista

Articulo

Indicadores

Links relacionados

  • No hay artículos similaresSimilares en SciELO

Compartir


Revista mexicana de astronomía y astrofísica

versión impresa ISSN 0185-1101

Resumen

GALINDO TREJO, J.. MHD Stability of a Solar Prominence Embedded in an External Vertical Magnetic Field. Rev. mex. astron. astrofis [online]. 2006, vol.42, n.1, pp.89-98. ISSN 0185-1101.

We examine the linear MHD-stability of a solar quiescent prominence described by the two-dimensional model of Osherovich (1989). This equilibrium model takes into account explicitly the influence of an external vertical magnetic field so that the prominence can be situated on the boundary between two regions of opposite magnetic polarity. We analyze its stability against perturbations within ideal MHD using a numerical method based on the Energy Principle of Bernstein et al. (1958). In our study specific cases of physical parameters observed in quiescent prominence are considered. For completeness we present as well results for other parameters which may perhaps be applicable to solar-type stars.

Palabras llave : MHD [WAVES]; SUN [OSCILLATIONS]; SUN [PROMINENCES].

        · resumen en Español     · texto en Inglés     · Inglés ( pdf )

 

Creative Commons License Todo el contenido de esta revista, excepto dónde está identificado, está bajo una Licencia Creative Commons