Modelling solar atmospheric gravity oscillation modes

Details Modelling solar atmospheric gravity oscillation modes Modelling solar atmospheric gravity oscillation modes

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008an....329..503p&link_type=abstract

Astronomische Nachrichten, Vol.329, Issue 5, p.503

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1

Hydrodynamics, Sun: Atmosphere, Sun: Helioseismology, Sun: Interior, Sun: Oscillations, Waves

Scientific paper

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.

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