Tidal dissipation in stars and giant planets
GI Ogilvie - Annual Review of Astronomy and Astrophysics, 2014 - annualreviews.org
Astrophysical fluid bodies that orbit close to one another induce tidal distortions and flows
that are subject to dissipative processes. The spin and orbital motions undergo a coupled …
that are subject to dissipative processes. The spin and orbital motions undergo a coupled …
Tidal dissipation in giant planets
Tidal interactions between moons and planets can have major effects on the orbits, spins,
and thermal evolution of the moons. In the Saturn system, tidal dissipation in the planet …
and thermal evolution of the moons. In the Saturn system, tidal dissipation in the planet …
Solar inertial modes: Observations, identification, and diagnostic promise
The oscillations of a slowly rotating star have long been classified into spheroidal and
toroidal modes. The spheroidal modes include the well-known 5-min acoustic modes used …
toroidal modes. The spheroidal modes include the well-known 5-min acoustic modes used …
Theory of solar oscillations in the inertial frequency range: Amplitudes of equatorial modes from a nonlinear rotating convection simulation
Context. Several types of inertial modes have been detected on the Sun. Properties of these
inertial modes have been studied in the linear regime, but have not been studied in …
inertial modes have been studied in the linear regime, but have not been studied in …
Effect of the rotation and tidal dissipation history of stars on the evolution of close-in planets
Since 20 years, a large population of close-in planets orbiting various classes of low-mass
stars (from M-type to A-type stars) has been discovered. In such systems, the dissipation of …
stars (from M-type to A-type stars) has been discovered. In such systems, the dissipation of …
Theory of solar oscillations in the inertial frequency range: Linear modes of the convection zone
Context. Several types of global-scale inertial modes of oscillation have been observed on
the Sun. These include the equatorial Rossby modes, critical-latitude modes, and high …
the Sun. These include the equatorial Rossby modes, critical-latitude modes, and high …
First evidence of inertial modes in γ Doradus stars: The core rotation revealed
RM Ouazzani, F Lignières, MA Dupret… - Astronomy & …, 2020 - aanda.org
The advent of space photometry with CoRoT and Kepler has allowed for the gathering of
exquisite and extensive time series for a wealth of main-sequence stars, including γ …
exquisite and extensive time series for a wealth of main-sequence stars, including γ …
Variation of tidal dissipation in the convective envelope of low-mass stars along their evolution
S Mathis - Astronomy & Astrophysics, 2015 - aanda.org
Context. Since 1995, more than 1500 exoplanets have been discovered around a wide
variety of host stars (from M-to A-type stars). Tidal dissipation in stellar convective envelopes …
variety of host stars (from M-to A-type stars). Tidal dissipation in stellar convective envelopes …
Tidally Excited Inertial Waves in Stars and Planets: Exploring the Frequency-dependent and Averaged Dissipation with Nonlinear Simulations
We simulate the nonlinear hydrodynamical evolution of tidally excited inertial waves in
convective envelopes of rotating stars and giant planets modeled as spherical shells …
convective envelopes of rotating stars and giant planets modeled as spherical shells …
Identification of inertial modes in the solar convection zone
The observation of global acoustic waves (p modes) in the Sun has been key to unveiling its
internal structure and dynamics. A different kind of wave, known as sectoral Rossby modes …
internal structure and dynamics. A different kind of wave, known as sectoral Rossby modes …