Forecast of solar activity based on mean-field dynamo model and neural network
Fuente:
arXiv
Guardado en:
| Autores principales: | Kleeorin, Nathan, Kuzanyan, Kirill, Safiullin, Nikolai, Rogachevskii, Igor, Obridko, Vladimir, Porshnev, Sergey, Stepanov, Rodion |
|---|---|
| Formato: | Preprint |
| Publicado: |
2024
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
Ejemplares similares
Magnetic fields of low-mass main sequences stars: Nonlinear dynamo theory and mean-field numerical simulations
por: Kleeorin, N., et al.
Publicado: (2023)
por: Kleeorin, N., et al.
Publicado: (2023)
Budget equations and astrophysical nonlinear mean-field dynamos
por: Rogachevskii, I., et al.
Publicado: (2023)
por: Rogachevskii, I., et al.
Publicado: (2023)
Alpha effect and dynamo in density-stratified turbulence with large-scale shear: applications to protoplanetary discs and astrophysical clouds
por: Rogachevskii, Igor, et al.
Publicado: (2025)
por: Rogachevskii, Igor, et al.
Publicado: (2025)
Solar poloidal magnetic field generation rate from observations and mean-field dynamos
por: Pipin, V. V.
Publicado: (2024)
por: Pipin, V. V.
Publicado: (2024)
Theory of the kinetic helicity effect on turbulent diffusion of magnetic and scalar fields
por: Rogachevskii, Igor, et al.
Publicado: (2025)
por: Rogachevskii, Igor, et al.
Publicado: (2025)
Large-scale clustering of inertial particles in a rotating, stratified and inhomogeneous turbulence
por: Kleeorin, Nathan, et al.
Publicado: (2025)
por: Kleeorin, Nathan, et al.
Publicado: (2025)
Characterizing the solar cycle variability using nonlinear time series analysis at different amounts of dynamo supercriticality: Solar dynamo is not highly supercritical
por: Ghosh, Aparup, et al.
Publicado: (2024)
por: Ghosh, Aparup, et al.
Publicado: (2024)
The solar dynamo begins near the surface
por: Vasil, Geoffrey M, et al.
Publicado: (2024)
por: Vasil, Geoffrey M, et al.
Publicado: (2024)
Long-term evolution of solar activity and prediction of the following solar cycles
por: Luo, Peixin, et al.
Publicado: (2024)
por: Luo, Peixin, et al.
Publicado: (2024)
Disentangling the solar activity-solar wind predictive causality at Space Climate scales
por: Reda, Raffaele, et al.
Publicado: (2023)
por: Reda, Raffaele, et al.
Publicado: (2023)
Solar cycle variability induced by stochastic fluctuations of BMR properties and at different amounts of dynamo supercriticality
por: Kumar, Pawan
Publicado: (2024)
por: Kumar, Pawan
Publicado: (2024)
On the estimation of solar wind velocity under varying solar activity conditions using Akatsuki measurements
por: Aggarwal, Keshav, et al.
Publicado: (2025)
por: Aggarwal, Keshav, et al.
Publicado: (2025)
New insights from cross-correlation studies between solar activity indices and cosmic-ray flux during Forbush decrease events
por: Savić, Mihailo, et al.
Publicado: (2026)
por: Savić, Mihailo, et al.
Publicado: (2026)
Near subsonic solar wind outflow from an active region
por: Ervin, Tamar, et al.
Publicado: (2024)
por: Ervin, Tamar, et al.
Publicado: (2024)
Identifying coronal sources of L1 solar wind disturbances using the Fisk heliospheric magnetic field and potential field extrapolations during three solar minima
por: Steyn, P. J., et al.
Publicado: (2024)
por: Steyn, P. J., et al.
Publicado: (2024)
Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical
por: Wavhal, Sanket, et al.
Publicado: (2025)
por: Wavhal, Sanket, et al.
Publicado: (2025)
Active regions and the large-scale magnetic field of solar cycle 24
por: Tähtinen, Ismo, et al.
Publicado: (2026)
por: Tähtinen, Ismo, et al.
Publicado: (2026)
Long-term variation of the solar polar magnetic fields at different latitudes
por: Yang, Shuhong, et al.
Publicado: (2024)
por: Yang, Shuhong, et al.
Publicado: (2024)
Observation and modeling of complex transient structure in heliosphere followed by geomagnetic storm on May 10-11, 2024
por: Rodkin, Denis, et al.
Publicado: (2025)
por: Rodkin, Denis, et al.
Publicado: (2025)
Addressing the open flux problem with a non-spherical solar coronal magnetic field model
por: Wu, Ziqi, et al.
Publicado: (2026)
por: Wu, Ziqi, et al.
Publicado: (2026)
Refinement of global coronal and interplanetary magnetic field extrapolations constrained by remote-sensing and in-situ observations at the solar minimum
por: Shi, Guanglu, et al.
Publicado: (2024)
por: Shi, Guanglu, et al.
Publicado: (2024)
EMISSA: Exploring millimetre indicators of solar-stellar activity III. Comparison of Ca II indices and millimetre continua in a 3D model atmosphere
por: Pandit, Sneha, et al.
Publicado: (2024)
por: Pandit, Sneha, et al.
Publicado: (2024)
The differences in the origination and properties of the near-Earth solar wind between solar cycles 23 and 24
por: Shi, Xinzheng, et al.
Publicado: (2024)
por: Shi, Xinzheng, et al.
Publicado: (2024)
The solar cycle 25 multi-spacecraft solar energetic particle event catalog of the SERPENTINE project
por: Dresing, N., et al.
Publicado: (2024)
por: Dresing, N., et al.
Publicado: (2024)
Estimating solar radiation environment extremes
por: Herbst, Konstantin, et al.
Publicado: (2025)
por: Herbst, Konstantin, et al.
Publicado: (2025)
Uniturbulence and Alfven wave solar model
por: Van Doorsselaere, Tom, et al.
Publicado: (2025)
por: Van Doorsselaere, Tom, et al.
Publicado: (2025)
Modeling HMI observables for the study of solar oscillations
por: Fournier, D., et al.
Publicado: (2025)
por: Fournier, D., et al.
Publicado: (2025)
Detection asymmetry in solar energetic particle events
por: Dalla, S., et al.
Publicado: (2024)
por: Dalla, S., et al.
Publicado: (2024)
Chromospheric dynamics and turbulence regulate the solar FIP effect
por: To, Andy S. H., et al.
Publicado: (2026)
por: To, Andy S. H., et al.
Publicado: (2026)
Tracking solar radio bursts using Bayesian multilateration
por: Cañizares, L. A., et al.
Publicado: (2024)
por: Cañizares, L. A., et al.
Publicado: (2024)
Alfvén wave propagation, reflection and trapping in the solar wind
por: Kumar, Anmol, et al.
Publicado: (2025)
por: Kumar, Anmol, et al.
Publicado: (2025)
Estimating uncertainties in the back-mapping of the fast solar wind
por: Koukras, Alexandros, et al.
Publicado: (2022)
por: Koukras, Alexandros, et al.
Publicado: (2022)
Emergence of two inertial sub-ranges in solar wind turbulence: dependence on heliospheric distance and solar activity
por: Mondal, Shiladittya, et al.
Publicado: (2024)
por: Mondal, Shiladittya, et al.
Publicado: (2024)
The role of photospheric magnetic flux diffusion in initiation of solar eruptions
por: Bian, Xinkai, et al.
Publicado: (2025)
por: Bian, Xinkai, et al.
Publicado: (2025)
Forecasting and Analysis of Solar Energetic Particle Radiation Storms
por: Malandraki, Olga, et al.
Publicado: (2025)
por: Malandraki, Olga, et al.
Publicado: (2025)
Evolution of MHD turbulence in the expanding solar wind: residual energy and intermittency
por: Shi, Chen, et al.
Publicado: (2023)
por: Shi, Chen, et al.
Publicado: (2023)
Multi-spacecraft observations of the decay phase of solar energetic particle events
por: Hyndman, R. A., et al.
Publicado: (2024)
por: Hyndman, R. A., et al.
Publicado: (2024)
The evolution of coronal shock wave properties and their relation with solar energetic particles
por: Jarry, Manon, et al.
Publicado: (2024)
por: Jarry, Manon, et al.
Publicado: (2024)
Towards advanced forecasting of solar energetic particle events with the PARASOL model
por: Afanasiev, Alexandr, et al.
Publicado: (2024)
por: Afanasiev, Alexandr, et al.
Publicado: (2024)
Straight outta photosphere: Open solar flux without coronal modeling
por: Tähtinen, Ismo, et al.
Publicado: (2024)
por: Tähtinen, Ismo, et al.
Publicado: (2024)
Ejemplares similares
-
Magnetic fields of low-mass main sequences stars: Nonlinear dynamo theory and mean-field numerical simulations
por: Kleeorin, N., et al.
Publicado: (2023) -
Budget equations and astrophysical nonlinear mean-field dynamos
por: Rogachevskii, I., et al.
Publicado: (2023) -
Alpha effect and dynamo in density-stratified turbulence with large-scale shear: applications to protoplanetary discs and astrophysical clouds
por: Rogachevskii, Igor, et al.
Publicado: (2025) -
Solar poloidal magnetic field generation rate from observations and mean-field dynamos
por: Pipin, V. V.
Publicado: (2024) -
Theory of the kinetic helicity effect on turbulent diffusion of magnetic and scalar fields
por: Rogachevskii, Igor, et al.
Publicado: (2025)