Anti-correlated Coupling p-Modes

Details Anti-correlated Coupling p-Modes Anti-correlated Coupling p-Modes

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sp31a09r&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SP31A-09

Astronomy and Astrophysics

Astrophysics

7500 Solar Physics, Astrophysics, And Astronomy, 7522 Helioseismology, 7544 Stellar Interiors And Dynamo Theory

Scientific paper

Using data from the MDI instrument and the GONG project we demonstrate that there exists an excess of anti-correlated 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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