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Cited article:
Damien Fournier , Laurent Gizon , Laura Hyest
A&A, 664 (2022) A6
Published online: 2022-08-04
This article has been cited by the following article(s):
12 articles
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The Sun’s differential rotation is controlled by high-latitude baroclinically unstable inertial modes
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A Linear Model for Inertial Modes in a Differentially Rotating Sun
Jishnu Bhattacharya, Chris S. Hanson, Shravan M. Hanasoge and Katepalli R. Sreenivasan The Astrophysical Journal 965 (1) 55 (2024) https://doi.org/10.3847/1538-4357/ad226c
Influence of the magnetic field and the mean flow configuration on spatial structure and growth rate of normal modes
Vladimir Mordvinov, Elena Devyatova and Vladimir Tomozov Solar-Terrestrial Physics 9 (4) 123 (2023) https://doi.org/10.12737/stp-94202315
Observed Power and Frequency Variations of Solar Rossby Waves with Solar Cycles
M. Waidele and Junwei Zhao The Astrophysical Journal Letters 954 (1) L26 (2023) https://doi.org/10.3847/2041-8213/acefd0
Influence of the magnetic field and the mean flow configuration on spatial structure and growth rate of normal modes
Vladimir Mordvinov, Elena Devyatova and Vladimir Tomozov Solnechno-Zemnaya Fizika 134 (2023) https://doi.org/10.12737/szf-94202315
Interaction of solar inertial modes with turbulent convection
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Theory of solar oscillations in the inertial frequency range: Linear modes of the convection zone
Yuto Bekki, Robert H. Cameron and Laurent Gizon Astronomy & Astrophysics 662 A16 (2022) https://doi.org/10.1051/0004-6361/202243164
Theory of solar oscillations in the inertial frequency range: Amplitudes of equatorial modes from a nonlinear rotating convection simulation
Yuto Bekki, Robert H. Cameron and Laurent Gizon Astronomy & Astrophysics 666 A135 (2022) https://doi.org/10.1051/0004-6361/202244150