Acoustic oscillations in a field-free cavity under solar small-scale bipolar magnetic canopy

Observations show the increase of high-frequency wave power near magnetic network cores and active regions in the solar lower atmosphere. This phenomenon can be explained by the interaction of acoustic waves with a magnetic field. We consider small-scale, bipolar, magnetic field canopy structure...

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Bibliographic Details
Main Authors: D. Kuridze, T. V. Zaqarashvili, B. M. Shergelashvili, S. Poedts
Format: Article
Language:English
Published: Copernicus Publications 2008-10-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/26/2983/2008/angeo-26-2983-2008.pdf
Description
Summary:Observations show the increase of high-frequency wave power near magnetic network cores and active regions in the solar lower atmosphere. This phenomenon can be explained by the interaction of acoustic waves with a magnetic field. We consider small-scale, bipolar, magnetic field canopy structure near the network cores and active regions overlying field-free cylindrical cavities of the photosphere. Solving the plasma equations we get the analytical dispersion relation of acoustic oscillations in the field-free cavity area. We found that the <I>m</I>=1 mode, where <I>m</I> is azimuthal wave number, cannot be trapped under the canopy due to energy leakage upwards. However, higher (<I>m</I>&ge;2) harmonics can be easily trapped leading to the observed acoustic power halos under the canopy.
ISSN:0992-7689
1432-0576