
doi: 10.1086/322363
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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