Structure of horizontal energy fluxes of five-minute oscillations

Details Structure of horizontal energy fluxes of five-minute oscillations Structure of horizontal energy fluxes of five-minute oscillations

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979azh....56..854z&link_type=abstract

Astronomicheskii Zhurnal, vol. 56, July-Aug. 1979, p. 854-861. In Russian.

Astronomy and Astrophysics

Astronomy

Magnetohydrodynamic Waves, Solar Atmosphere, Solar Oscillations, Solar Spectra, Anisotropy, Astronomical Spectroscopy, Chromosphere, Spectral Energy Distribution, Wave Propagation

Scientific paper

The structure of horizontal wave fluxes is investigated theoretically for the global and local mechanisms of producing the five-minute solar oscillations. Both distributed absorption and the presence of point energy sinks are taken into account. Observations of the five-minute oscillations in the Ba II line at 4554 + 0.05 A are discussed which indicate regular large-scale and irregular small-scale horizontal wave-flux structures. The possibility is considered that the large-scale structures occur as a result of single-mode production with a regular distribution of local wave-energy sinks.

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