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Inertial modes trapped in the solar convective envelope

Published online by Cambridge University Press:  03 August 2017

W. Dziembowski ,
A. Kosovichev  and
M. Kozlowski.
W. Dziembowski
Affiliation:
N. Copernicus Astronomical Center, ul. Bartycka 18, 00-716 Warszawa, Poland
A. Kosovichev
Affiliation:
N. Copernicus Astronomical Center, ul. Bartycka 18, 00-716 Warszawa, Poland
M. Kozlowski.
Affiliation:
N. Copernicus Astronomical Center, ul. Bartycka 18, 00-716 Warszawa, Poland

Abstract

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Due to their efficient trapping in the outer layers such modes may reach observable amplitudes of the order of 1–10 m/s, even if their energies are as those of the “five minute” oscillations. The modes that are most likely to be seen correspond to the lowest radial orders.

The paper will be published in Acta Astronomica.

Type
Chapter 2: Theory of Solar Oscillations
Information
Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 117
Copyright
Copyright © Reidel 1988