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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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
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spelling doaj-dd620130ae494bc18794ce838b5865a52020-11-24T23:37:49ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762008-10-01262983298910.5194/angeo-26-2983-2008Acoustic oscillations in a field-free cavity under solar small-scale bipolar magnetic canopyD. Kuridze0T. V. Zaqarashvili1B. M. Shergelashvili2B. M. Shergelashvili3S. Poedts4Georgian National Astrophysical Observatory (Abastumani Astrophysical Observatory), Al. Kazbegi ave. 2a, 0160 Tbilisi, GeorgiaGeorgian National Astrophysical Observatory (Abastumani Astrophysical Observatory), Al. Kazbegi ave. 2a, 0160 Tbilisi, GeorgiaGeorgian National Astrophysical Observatory (Abastumani Astrophysical Observatory), Al. Kazbegi ave. 2a, 0160 Tbilisi, GeorgiaInstitute for Theoretical Physics, K.U. Leuven, Celestijnenlaan 200 D, 3001, Leuven, BelgiumCenter for Plasma Astrophysics, K.U.Leuven, 200 B, 3001, Leuven, BelgiumObservations 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.https://www.ann-geophys.net/26/2983/2008/angeo-26-2983-2008.pdf
collection DOAJ
language English
format Article
sources DOAJ
author D. Kuridze
T. V. Zaqarashvili
B. M. Shergelashvili
B. M. Shergelashvili
S. Poedts
spellingShingle D. Kuridze
T. V. Zaqarashvili
B. M. Shergelashvili
B. M. Shergelashvili
S. Poedts
Acoustic oscillations in a field-free cavity under solar small-scale bipolar magnetic canopy
Annales Geophysicae
author_facet D. Kuridze
T. V. Zaqarashvili
B. M. Shergelashvili
B. M. Shergelashvili
S. Poedts
author_sort D. Kuridze
title Acoustic oscillations in a field-free cavity under solar small-scale bipolar magnetic canopy
title_short Acoustic oscillations in a field-free cavity under solar small-scale bipolar magnetic canopy
title_full Acoustic oscillations in a field-free cavity under solar small-scale bipolar magnetic canopy
title_fullStr Acoustic oscillations in a field-free cavity under solar small-scale bipolar magnetic canopy
title_full_unstemmed Acoustic oscillations in a field-free cavity under solar small-scale bipolar magnetic canopy
title_sort acoustic oscillations in a field-free cavity under solar small-scale bipolar magnetic canopy
publisher Copernicus Publications
series Annales Geophysicae
issn 0992-7689
1432-0576
publishDate 2008-10-01
description 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.
url https://www.ann-geophys.net/26/2983/2008/angeo-26-2983-2008.pdf
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