Imagen de Portada

Excitation of Inertial Modes in 3D Simulations of Rotating Convection in Planets and Stars

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Fuentes, J. R., Barik, Ankit, Fuller, Jim
Formato:	Preprint
Publicado:	2025
Materias:	Solar and Stellar Astrophysics Earth and Planetary Astrophysics Fluid Dynamics
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Viscous Dissipation and Dynamics in Simulations of Rotating, Stratified Plane-layer Convection
por: Lance, Simon R. W., et al.
Publicado: (2024)

3D Simulations of Semiconvection in Spheres: Turbulent Mixing and Layer Formation
por: Fuentes, J. R.
Publicado: (2025)

Transition to turbulence in the wide-gap spherical Couette system
por: Barik, Ankit, et al.
Publicado: (2024)

Influence of Boundary Conditions and Heating Modes on the Onset of Columnar Convection in Rotating Spherical Shells
por: Seeley, William, et al.
Publicado: (2025)

Excitation and Damping of Oscillation Modes in Gaseous Planets
por: Fuller, Jim, et al.
Publicado: (2026)

Diffusion-Free Dynamics in Rotating Spherical Shell Convection Driven By Internal Heating and Cooling
por: Lewis, Neil T., et al.
Publicado: (2025)

Predicting the Slowing of Stellar Differential Rotation by Instability-Driven Turbulence
por: Tripathi, B., et al.
Publicado: (2024)

Scaling with the Stars: The emergence of marginal stability in low Prandtl number turbulence
por: Shah, Kasturi
Publicado: (2024)

Classical 1/3 Nusselt number scaling in highly turbulent compressible convection
por: Tiwari, Harshit, et al.
Publicado: (2025)

Interplay between tidal flows and magnetic fields in nonlinear simulations of stellar and planetary convective envelopes
por: Astoul, Aurélie, et al.
Publicado: (2025)

The stability of propagating plane inertial waves in rotating fluids
por: Skoutnev, Valentin, et al.
Publicado: (2025)

Run-away transition to turbulent strong-field dynamo
por: Guseva, Anna, et al.
Publicado: (2024)

On the stability of viscous Riemann ellipsoids
por: Labarbe, Joris
Publicado: (2026)

"Halfway to Rayleigh" and other Insights to the Rossby Wave Instability
por: Chang, Eonho, et al.
Publicado: (2024)

Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows
por: Lynch, Elliot M., et al.
Publicado: (2024)

A high resolution simulation of protoplanetary disk turbulence driven by the vertical shear instability
por: Shariff, Karim, et al.
Publicado: (2024)

The role of magnetic boundaries in kinematic and self-consistent magnetohydrodynamic simulations of precession-driven dynamo action in a closed cylinder
por: Giesecke, André, et al.
Publicado: (2024)

Large-scale clustering of inertial particles in a rotating, stratified and inhomogeneous turbulence
por: Kleeorin, Nathan, et al.
Publicado: (2025)

PT and anti-PT symmetries for astrophysical waves
por: Leclerc, Armand, et al.
Publicado: (2024)

Fingering convection in a spherical shell
por: Tassin, T., et al.
Publicado: (2023)

A physical picture for the acoustic resonant drag instability
por: Magnan, Nathan, et al.
Publicado: (2024)

Dynamo action driven by precessional turbulence
por: Kumar, V., et al.
Publicado: (2023)

Strong and weak dynamo regimes in Taylor-Couette flows
por: Mishra, A., et al.
Publicado: (2025)

Pade: A code for protoplanetary disk turbulence based on Pade differencing
por: Shariff, Karim
Publicado: (2024)

Magnetic Activity Cycles and Rotation in Planet-hosting and Non-hosting Solar-type Stars
por: Boulkaboul, Amina, et al.
Publicado: (2026)

Modeling dust dynamics in OpenGadget3 -- I. SPH implementation of the One-Fluid model
por: Tedeschi-Prades, Giovanni, et al.
Publicado: (2025)

An Energy Perspective of Core Erosion in Gas Giant Planets
por: Fuentes, J. R., et al.
Publicado: (2025)

Non-linear evolution of the horizontal shear instability in stratified rotating fluids under the complete Coriolis acceleration
por: Moisset, Camille, et al.
Publicado: (2025)

Understanding hydrodynamical wave-driven shear mixing in stellar radiation zones. Looking in the mirror of the dyapicnal oceanic mixing
por: Mathis, Stéphane
Publicado: (2026)

Flares, Rotation, Activity Cycles and a Magnetic Star-Planet Interaction Hypothesis for the Far Ultraviolet Emission of GJ 436
por: Loyd, R. O. Parke, et al.
Publicado: (2023)

Dynamics of Binary Planets within Star Clusters
por: Huang, Yukun, et al.
Publicado: (2024)

C3PO III: On the Lithium Signatures Following Planet Engulfment by Stars
por: Sun, Qinghui, et al.
Publicado: (2024)

The Dynamic Inner Disk of a Planet Forming Star
por: Setterholm, Benjamin R., et al.
Publicado: (2025)

A Small Brown Dwarf in an Aligned Orbit around a Young, Fully-Convective M Star
por: Brady, M., et al.
Publicado: (2024)

Distinct Rotational Evolution of Giant Planets and Brown Dwarf Companions
por: Hsu, Chih-Chun, et al.
Publicado: (2026)

Observable Metal Pollution in Main-Sequence Stars: Simulations of Rocky Planets Engulfed by Stars in the $0.5$ to $1.4$ M$_\odot$ Range
por: Lane, Kaitlyn T., et al.
Publicado: (2026)

A Radio Search for Star-Planet Interaction in TOI-540 and SPECULOOS-3
por: Ceballos, Kevin N. Ortiz, et al.
Publicado: (2025)

Morphological Regimes of Rotating Moist Convection
por: Powers, Whitney T., et al.
Publicado: (2025)

No Planet around the K Giant Star 42 Draconis
por: Hatzes, Artie P., et al.
Publicado: (2025)

Star-Planet Interactions in the Radio Domain: Prospect for Their Detection
por: Zarka, Philippe
Publicado: (2024)