Enhancement of wave transmissions in multiple radiative and convective zones
arXiv:2102.12018 · doi:10.1017/jfm.2021.178
Abstract
In this paper, we study wave transmission in a rotating fluid with multiple alternating convectively stable and unstable layers. We have discussed wave transmissions in two different circumstances: cases where the wave is propagative in each layer and cases where wave tunneling occurs. We find that efficient wave transmission can be achieved by `resonant propagation' or `resonant tunneling', even when stable layers are strongly stratified, and we call this phenomenon `enhanced wave transmission'. Enhanced wave transmission only occurs when the total number of layers is odd (embedding stable layers are alternatingly embedded within clamping convective layers, or vise versa). For wave propagation, the occurrence of enhanced wave transmission requires that clamping layers have similar properties, the thickness of each clamping layer is close to a multiple of the half wavelength of the corresponding propagative wave, and the total thickness of embedded layers is close to a multiple of the half wavelength of the corresponding propagating wave (resonant propagation). For wave tunneling, we have considered two cases: tunneling of gravity waves and tunneling of inertial waves. In both cases, efficient tunneling requires that clamping layers have similar properties, the thickness of each embedded layer is much smaller than the corresponding e-folding decay distance, and the thickness of each clamping layer is close to a multiple-and-a-half of half wavelength (resonant tunneling).
arXiv commentaccepted to J. Fluid Mech
References in corpus (21)
- Tidal dissipation in rotating giant planets
- Angular Momentum Transport in Stellar Interiors
- A new vision on giant planet interiors: the impact of double diffusive convection
- Internal Gravity Waves in Massive Stars: Angular Momentum Transport
- Inertial waves in a rotating spherical shell: attractors and asymptotic spectrum
- Internal Gravity Waves Modulate the Apparent Misalignment of Exoplanets around Hot Stars
- Saturn Ring Seismology: Evidence for Stable Stratification in the Deep Interior of Saturn
- Origin of Tidal Dissipation in Jupiter: II. the Value of Q
- A new model for mixing by double-diffusive convection (semi-convection): I. The conditions for layer formation
- Dynamical Tides in Rotating Planets and Stars
- A new model for mixing by double-diffusive convection (semi-convection). II. The transport of heat and composition through layers
- Origin of Tidal Dissipation in Jupiter: I. Properties of Inertial-Mode
- Angular momentum redistribution by mixed modes in evolved low-mass stars. II. Spin-down of the core of red giants induced by mixed modes
- Can plume-induced internal gravity waves regulate the core rotation of subgiant stars?
- Angular momentum redistribution by mixed modes in evolved low-mass stars. I. Theoretical formalism
- Main Sequence Evolution with Layered Semiconvection
- Wave propagation in semi-convective regions of giant planets
- The Properties of G-modes in Layered Semi-Convection
- The Interaction Of Multiple Convection Zones In A-type Stars
- Inertial and gravity wave transmissions near radiative-convective boundaries
- Wave reflection and transmission at interface of convective and stably stratified regions in a rotating star or planet