Modelling solar atmospheric gravity oscillation modes

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7 Citations (Scopus)


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.
Original languageEnglish
Pages (from-to)503-507
JournalAstronomische Nachrichten
Issue number5
Publication statusPublished - Jun 2008


  • hydrodynamics
  • Sun: atmosphere
  • Sun: helioseismology
  • Sun: interior
  • Sun: oscillations
  • waves


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