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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2008-10-01
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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>≥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>≥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 |
work_keys_str_mv |
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