Integrated light and velocity of solar G modes oscillations

Details Integrated light and velocity of solar G modes oscillations Integrated light and velocity of solar G modes oscillations

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286..387p&link_type=abstract

In ESA, Seismology of the Sun and Sun-Like Stars p 387-391 (SEE N89-25819 19-92)

Physics

2

Solar Constant, Solar Gravitation, Solar Oscillations, Adiabatic Conditions, Amplitude Distribution Analysis, Nonadiabatic Conditions, Spatial Filtering, Velocity Distribution

Scientific paper

The properties of the integrated intensity and velocity variations of the solar gravity modes for different spatial filters are studied in the adiabatic and nonadiabatic cases in the frequency range 40 to 120 micro Hz. Predicted amplitudes are given assuming equipartition of energy between the modes. As far as the intensity is concerned, a lack of amplitude is pointed out around 60 micro Hz, which should have implications on the whole disk VIRGO and ground based observations.

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