Modelling solar atmospheric gravity oscillation modes | Zendy

Pintér B. | Zendy

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Modelling solar atmospheric gravity oscillation modes

Author(s) -

Pintér B.

Publication year - 2008

Publication title -

astronomische nachrichten

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 0.394

H-Index - 63

eISSN - 1521-3994

pISSN - 0004-6337

DOI - 10.1002/asna.200710985

Subject(s) - physics , oscillation (cell signaling) , atmosphere (unit) , mode (computer interface) , plane (geometry) , atmospheric pressure , computational physics , normal mode , mechanics , meteorology , geometry , acoustics , chemistry , vibration , mathematics , computer science , operating system , biochemistry

Solar oscillations are investigated in a one‐dimensional hydrodynamic plane‐parallel model with an atmosphere. Besides the acoustic pressure (p) modes, the fundamental (f) and Lamb mode, another set of eigenmodes, a group of atmospheric gravity (g) modes, is found in the low‐frequency region of the spectrum. Their frequencies and spatial behaviour are studied. (© 2008 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)

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