Temporal Variation of Solar Equatorial Rossby Modes with Azimuthal Orders $6\leq m \leq 10$
Fuente:
arXiv
Guardado en:
| Autores principales: | Lekshmi, B., Gizon, Laurent, Jain, Kiran, Liang, Zhi-Chao, Philidet, Jordan |
|---|---|
| Formato: | Preprint |
| Publicado: |
2024
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
Ejemplares similares
Temporal variations of solar inertial mode parameters from GONG (2002--2024) and HMI (2010--2024): Rossby modes ($3 \leq m \leq 16 $) and $m=1$ high-latitude mode
por: Lekshmi, B, et al.
Publicado: (2026)
por: Lekshmi, B, et al.
Publicado: (2026)
Solar Inertial Modes
por: Gizon, Laurent, et al.
Publicado: (2024)
por: Gizon, Laurent, et al.
Publicado: (2024)
Doppler velocity of $m=1$ high-latitude inertial mode over the last five sunspot cycles
por: Liang, Zhi-Chao, et al.
Publicado: (2024)
por: Liang, Zhi-Chao, et al.
Publicado: (2024)
Oscillations of the solar photospheric magnetic field caused by the m = 1 high-latitude inertial mode
por: Heinemann, Stephan G., et al.
Publicado: (2025)
por: Heinemann, Stephan G., et al.
Publicado: (2025)
Dynamics of Subsurface Flows in Solar Active Regions During the May 2024 Storm
por: Lekshmi, B, et al.
Publicado: (2025)
por: Lekshmi, B, et al.
Publicado: (2025)
Observations of eigenfunctions of solar inertial modes using local correlation tracking of magnetic features
por: Joshi, Neelanchal, et al.
Publicado: (2025)
por: Joshi, Neelanchal, et al.
Publicado: (2025)
The Initial mass function of field stars with mass $\leq$ 1 $M_{\odot}$ varies with metallicity
por: Qiu, Dan, et al.
Publicado: (2025)
por: Qiu, Dan, et al.
Publicado: (2025)
Structural Tilting and Depth-Dependent Behavior of Equatorial Rossby Waves
por: Vesa, Oana, et al.
Publicado: (2026)
por: Vesa, Oana, et al.
Publicado: (2026)
Towards inertial-mode helioseismology: Direct sensing of solar rotation at 75 deg latitude and 0.8 Rsun
por: Dey, Prithwitosh, et al.
Publicado: (2026)
por: Dey, Prithwitosh, et al.
Publicado: (2026)
The mean solar butterfly diagram and poloidal field generation rate at the surface of the Sun
por: Cloutier, Simon, et al.
Publicado: (2024)
por: Cloutier, Simon, et al.
Publicado: (2024)
The rush to the poles and the role of magnetic buoyancy in the solar dynamo
por: Cloutier, Simon, et al.
Publicado: (2024)
por: Cloutier, Simon, et al.
Publicado: (2024)
A new particle-based code for Lagrangian stochastic models applied to stellar turbulent convection
por: Philidet, J., et al.
Publicado: (2025)
por: Philidet, J., et al.
Publicado: (2025)
Probing Depth Variations of Solar Inertial Modes through Normal Mode Coupling
por: Mandal, Krishnendu, et al.
Publicado: (2024)
por: Mandal, Krishnendu, et al.
Publicado: (2024)
Long-Term Clustering Pattern of Solar Active Regions and Their Potential Connection with Magneto-Rossby Waves
por: Zhao, Junwei, et al.
Publicado: (2026)
por: Zhao, Junwei, et al.
Publicado: (2026)
Assessing the validity of the anelastic and Boussinesq approximations to model solar inertial modes
por: Mukhopadhyay, Suprabha, et al.
Publicado: (2025)
por: Mukhopadhyay, Suprabha, et al.
Publicado: (2025)
Effects of the radiative interior on solar inertial modes
por: Mukhopadhyay, Suprabha, et al.
Publicado: (2025)
por: Mukhopadhyay, Suprabha, et al.
Publicado: (2025)
Machine Learning-Based Characterization of Solar p-Mode Frequency Shifts during Solar Cycle 25
por: Jain, Rekha, et al.
Publicado: (2026)
por: Jain, Rekha, et al.
Publicado: (2026)
Extending the Asteroseismic Calibration of the Stellar Rossby Number
por: Metcalfe, Travis S., et al.
Publicado: (2024)
por: Metcalfe, Travis S., et al.
Publicado: (2024)
Effects of density stratification on Rossby waves in deep atmospheres
por: Blume, Catherine C., et al.
Publicado: (2025)
por: Blume, Catherine C., et al.
Publicado: (2025)
[X/Fe] Marks the Spot: Mapping Chemical Azimuthal Variations in the Galactic Disk with APOGEE
por: Hackshaw, Zoe, et al.
Publicado: (2024)
por: Hackshaw, Zoe, et al.
Publicado: (2024)
Combined Surface Flux Transport and Helioseismic Far-side Active Region Model (FARM)
por: Yang, Dan, et al.
Publicado: (2024)
por: Yang, Dan, et al.
Publicado: (2024)
Surface activity of a Rossby sequence of cool Hyades stars
por: Strassmeier, K. G., et al.
Publicado: (2025)
por: Strassmeier, K. G., et al.
Publicado: (2025)
Evaluating Solar Wind Forecast Using Magnetic Maps That Include Helioseismic Far-Side Information
por: Heinemann, Stephan G., et al.
Publicado: (2025)
por: Heinemann, Stephan G., et al.
Publicado: (2025)
Subsurface Flows in Active Regions with Peculiar Magnetic Configurations
por: Jain, Kiran, et al.
Publicado: (2023)
por: Jain, Kiran, et al.
Publicado: (2023)
Moderate Nesting and Cross-Equatorial Asymmetry of Active Regions in Solar Cycle 24
por: Norton, Aimee, et al.
Publicado: (2025)
por: Norton, Aimee, et al.
Publicado: (2025)
The Sun's differential rotation is controlled by high-latitude baroclinically unstable inertial modes
por: Bekki, Yuto, et al.
Publicado: (2024)
por: Bekki, Yuto, et al.
Publicado: (2024)
Asteroseismic calibration of the Rossby number and its connection to the stellar dynamo and fundamental properties
por: Bonanno, Alfio, et al.
Publicado: (2025)
por: Bonanno, Alfio, et al.
Publicado: (2025)
Testing the Rossby Paradigm: Weakened Magnetic Braking in early K-type Stars
por: Metcalfe, Travis S., et al.
Publicado: (2025)
por: Metcalfe, Travis S., et al.
Publicado: (2025)
Glitches in solar-like oscillating F-type stars: Possible contribution of non-linear terms
por: Deal, M., et al.
Publicado: (2024)
por: Deal, M., et al.
Publicado: (2024)
Temporal Variation of Flare Occurrence Rates via the Spot Evolution on the Sun and Solar-type Stars
por: Tokuno, Takato, et al.
Publicado: (2025)
por: Tokuno, Takato, et al.
Publicado: (2025)
Magnetohydrodynamic shallow water equations with the alpha effect: Rossby-dynamo waves in solar--stellar tachoclines
por: Zaqarashvili, T. V., et al.
Publicado: (2025)
por: Zaqarashvili, T. V., et al.
Publicado: (2025)
Time Variation of the Solar Tachocline
por: Basu, Sarbani, et al.
Publicado: (2024)
por: Basu, Sarbani, et al.
Publicado: (2024)
Temporal Variations in Asteroseismic Frequencies of KIC 6106415: Insights into the Solar-Stellar Activity from GOLF and Kepler Observations
por: Lombardi, Christopher J., et al.
Publicado: (2025)
por: Lombardi, Christopher J., et al.
Publicado: (2025)
Coriolis force acting on near-surface horizontal flows during simulations of flux emergence produces a tilt angle consistent with Joy's law on the Sun
por: Roland-Batty, William, et al.
Publicado: (2025)
por: Roland-Batty, William, et al.
Publicado: (2025)
A Scenario for Origin of Global 4 mHz Oscillations in Solar Corona
por: Xue, Li, et al.
Publicado: (2025)
por: Xue, Li, et al.
Publicado: (2025)
Variations in Dominant Wave Period in the Solar Atmosphere
por: Kayshap, Pradeep, et al.
Publicado: (2025)
por: Kayshap, Pradeep, et al.
Publicado: (2025)
Investigating Variations in Solar Differential Rotation by Helioseismology
por: Mandal, Krishnendu, et al.
Publicado: (2025)
por: Mandal, Krishnendu, et al.
Publicado: (2025)
Latitude-Dependent Time Variations of the Solar Tachocline
por: Basu, Sarbani, et al.
Publicado: (2026)
por: Basu, Sarbani, et al.
Publicado: (2026)
Assembling algorithm for Green's tensors and absorbing boundary conditions for Galbrun's equation in radial symmetry
por: Pham, Ha, et al.
Publicado: (2024)
por: Pham, Ha, et al.
Publicado: (2024)
Swaying oscillations in Rayleigh-Bénard convection cast new light on solar convection
por: Kupka, F., et al.
Publicado: (2025)
por: Kupka, F., et al.
Publicado: (2025)
Ejemplares similares
-
Temporal variations of solar inertial mode parameters from GONG (2002--2024) and HMI (2010--2024): Rossby modes ($3 \leq m \leq 16 $) and $m=1$ high-latitude mode
por: Lekshmi, B, et al.
Publicado: (2026) -
Solar Inertial Modes
por: Gizon, Laurent, et al.
Publicado: (2024) -
Doppler velocity of $m=1$ high-latitude inertial mode over the last five sunspot cycles
por: Liang, Zhi-Chao, et al.
Publicado: (2024) -
Oscillations of the solar photospheric magnetic field caused by the m = 1 high-latitude inertial mode
por: Heinemann, Stephan G., et al.
Publicado: (2025) -
Dynamics of Subsurface Flows in Solar Active Regions During the May 2024 Storm
por: Lekshmi, B, et al.
Publicado: (2025)