Imagen de Portada

Nonlinear evolution of unstable solar inertial modes: The case of viscous modes on a differentially rotating sphere

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Mushtaq, Muneeb, Fournier, Damien, Ayoub, Rama, Schmid, Peter J., Gizon, Laurent
Formato:	Preprint
Publicado:	2026
Materias:	Solar and Stellar Astrophysics Fluid Dynamics
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

The Sun's differential rotation is controlled by high-latitude baroclinically unstable inertial modes
por: Bekki, Yuto, et al.
Publicado: (2024)

Observations of eigenfunctions of solar inertial modes using local correlation tracking of magnetic features
por: Joshi, Neelanchal, et al.
Publicado: (2025)

Kelvin waves over a differentially rotating spherical shell
por: Boismard, T., et al.
Publicado: (2026)

Secondary small-scale dynamics of a Rayleigh-Taylor unstable solar prominence
por: Changmai, Madhurjya, et al.
Publicado: (2025)

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

Effects of the radiative interior on solar inertial modes
por: Mukhopadhyay, Suprabha, et al.
Publicado: (2025)

Towards inertial-mode helioseismology: Direct sensing of solar rotation at 75 deg latitude and 0.8 Rsun
por: Dey, Prithwitosh, et al.
Publicado: (2026)

The importance of Berry phase in solar acoustic modes
por: Leclerc, Armand, et al.
Publicado: (2025)

$Λ$ effect in rotating hydrodynamic convection
por: Käpylä, P. J.
Publicado: (2026)

Mathematical formulation of mode-to-mode energy transfers and energy fluxes in compressible turbulence
por: Singh, Dhananjay, et al.
Publicado: (2025)

Effects of rotation and surface forcing on deep stellar convection zones
por: Käpylä, Petri J.
Publicado: (2023)

Assessing the validity of the anelastic and Boussinesq approximations to model solar inertial modes
por: Mukhopadhyay, Suprabha, et al.
Publicado: (2025)

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

Inferring solar differential rotation and viscosity via passive imaging with inertial waves
por: Nguyen, Tram Thi Ngoc, et al.
Publicado: (2024)

Nonlinear wave damping by Kelvin-Helmholtz instability induced turbulence
por: Hillier, Andrew, et al.
Publicado: (2023)

Numerical simulations of oscillations for axisymmetric solar backgrounds with differential rotation and gravity
por: Pham, Ha, et al.
Publicado: (2025)

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

Effects of External Magnetic Fields on the Multi-mode Rayleigh-Taylor Instability
por: Bian, Xin, et al.
Publicado: (2025)

Oscillations of the solar photospheric magnetic field caused by the m = 1 high-latitude inertial mode
por: Heinemann, Stephan G., et al.
Publicado: (2025)

One-winged butterflies: mode selection for azimuthal magnetorotational instability by thermal convection
por: Mishra, A., et al.
Publicado: (2024)

Nonlinear interaction between dynamo-generated magnetic fields, mean flows and internal gravity waves in stellar stably-stratified layers: From 3D to 1D
por: Daniel, Florentin, et al.
Publicado: (2026)

Doppler velocity of $m=1$ high-latitude inertial mode over the last five sunspot cycles
por: Liang, Zhi-Chao, et al.
Publicado: (2024)

The solar dynamo begins near the surface
por: Vasil, Geoffrey M, et al.
Publicado: (2024)

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

Modelling the Solar Cycle Nonlinearities into the Algebraic Approach
por: Talafha, Mohammed H.
Publicado: (2025)

Data-driven discovery of the equations of turbulent convection
por: Wareing, Christopher J., et al.
Publicado: (2025)

New branch of the Tayler-Spruit dynamo in stellar radiative zones
por: Barrère, Paul, et al.
Publicado: (2026)

Helicity subgrid-scale models and their numerical validation
por: Yokoi, Nobumitsu, et al.
Publicado: (2026)

Towards a self-consistent model of the convective core boundary in upper main sequence stars. Part I: 2.5D and 3D simulations
por: Andrassy, R., et al.
Publicado: (2023)

Rayleigh-Taylor Unstable Flames: Thin and Thick
por: Hicks, Elizabeth P.
Publicado: (2026)

Modeling stellar convective transport with plumes : II. Transport Properties of Locally and Non-locally driven Convection
por: Masada, Youhei, et al.
Publicado: (2025)

On the possibility of chemically driven convection in red giants. Implications for the He-core flash and mixing above the Red Giant Branch Bump
por: Ocampo, M. Miguel, et al.
Publicado: (2026)

Small-Scale Dynamo for Full Spectrum of Hydrodynamic Turbulence in Kazantsev Model
por: Kitchatinov, Leonid
Publicado: (2026)

A new particle-based code for Lagrangian stochastic models applied to stellar turbulent convection
por: Philidet, J., et al.
Publicado: (2025)

Unstable gas flow in a flat channel under the influence of a transverse force field: self-oscillations of the jet
por: Korolkov, S. D., et al.
Publicado: (2024)

The Interaction between Solar Convection and Rotation
por: Chen, Haibin, et al.
Publicado: (2024)

Internally heated and fully compressible convection: flow morphology and scaling laws
por: Powers, Whitney T., et al.
Publicado: (2023)

Helicity oscillations in Rayleigh-Bénard convection of liquid metal in a cell with aspect ratio 0.5
por: Mitra, R., et al.
Publicado: (2024)

Compressible turbulent convection: The role of temperature-dependent thermal conductivity and dynamic viscosity
por: John, John Panickacheril, et al.
Publicado: (2024)

Transient and steady convection in two dimensions
por: Pandey, Ambrish, et al.
Publicado: (2025)