Spatial stratification of acoustic oscillations in the solar photosphere

Space-time variations of solar atmosphere parameters are derived by solving non-equilibrium radiation transfer problem. Acoustic oscillations were extracted using k − ω filtration of variations. In the lower photosphere there are evanescent remnants of underphotosphere oscillations; in the middle an...

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Veröffentlicht in:Кинематика и физика небесных тел
Datum:2005
ISSN:0233-7665
1. Verfasser: Stodilka, M.I.
Format: Artikel
Sprache:Englisch
Veröffentlicht: Головна астрономічна обсерваторія НАН України 2005
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Online Zugang:https://nasplib.isofts.kiev.ua/handle/123456789/79617
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Zitieren:Spatial stratification of acoustic oscillations in the solar photosphere / M.I. Stodilka // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 124-128. — Бібліогр.: 9 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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Zusammenfassung:Space-time variations of solar atmosphere parameters are derived by solving non-equilibrium radiation transfer problem. Acoustic oscillations were extracted using k − ω filtration of variations. In the lower photosphere there are evanescent remnants of underphotosphere oscillations; in the middle and high photosphere there are discrete sources of oscillations, which are excited by granule decay and formation of a new intergranule. The photosphere is penetrated by narrow “channels”, by which energy of fluctuations tunnels with minimal losses into the higher atmosphere layers; such “channels” arise mostly between ascending and descending flows. Particularities of the wave propagation in the solar atmosphere are determined by relationship between wavelength and the effective size of inhomogeneities.
ISSN:0233-7665