Anticorrelated Coupling p-Modes

Details Anticorrelated Coupling p-Modes Anticorrelated Coupling p-Modes

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001apj...559.1165r&link_type=abstract

The Astrophysical Journal, Volume 559, Issue 2, pp. 1165-1170.

Astronomy and Astrophysics

Astronomy

3

Convection, Methods: Data Analysis, Sun: Interior, Sun: Oscillations

Scientific paper

Using data from the Michelson Doppler Imager and the Global Oscillation Network Group project, we demonstrate that there exists an excess of anticorrelated power variations of pairs of solar p-modes. We find a possible explanation for this behavior in the influence of poloidal velocity fields, which may lead to coupling of p-modes that results in an energy redistribution among the solar oscillations.

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