Short period oscillations

Details Short period oscillations Short period oscillations

Jan 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...82..151d&link_type=abstract

(International Astronomical Union and Akademiia Nauk SSSR, Colloquium on Problems of Solar and Stellar Oscillations, 66th, Nauch

Physics

7

Solar Atmosphere, Solar Oscillations, Solar Spectra, Brightness, Chromosphere, Energy Transfer, Magnetohydrodynamic Waves, Photosphere, Solar Physics, Wave Propagation

Scientific paper

Oscillations of period shorter than 150 sec are nonuniformly distributed both over the solar surface and in time, concentrating in long bursts which preferentially occur in regions with strong, instantaneous downflow motion throughout the observed extent of the solar atmosphere. It is established that three well known solar phenomena, granulation and the photospheric and chromospheric p-modes, which have not been considered mutually related, are spatially coupled together under certain additional constraints with regard to temporal phase. This coupling produces a fourth phenomenon, either a rapid pulse or a short period burst.

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