Imagen de Portada

Observation-Based Iterative Map for Solar Cycles. II. The Gnevyshev-Ohl Rule and its Generation Mechanism

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Wang, Zi-Fan, Jiang, Jie, Wang, Jing-Xiu
Formato:	Preprint
Publicado:	2025
Materias:	Solar and Stellar Astrophysics
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Observation-Based Iterative Map for Solar Cycles. I. Nature of Solar Cycle Variability
por: Wang, Zi-Fan, et al.
Publicado: (2025)

Gnevyshev gap in the large-scale magnetic field
por: Obridko, V. N., et al.
Publicado: (2024)

Prediction of the Solar Polar Fields in 2026: An Unusually Weak Level Across the Last Five Solar Cycles
por: Wang, Ruihui, et al.
Publicado: (2025)

The Sun's Magnetic Power Spectra over Two Solar Cycles. \uppercase\expandafter{\romannumeral2}. Cycle Dependence of Active Region, Magnetic Network, and Their Relation
por: Luo, Yukun, et al.
Publicado: (2024)

Solar Surface Magnetic Field Simulation from 2010 to 2024 and Anomalous Southern Poleward Flux Transport in Cycle 24
por: Wang, Ruihui, et al.
Publicado: (2025)

Spectroscopic and Decade-long Photometric Observations of the Contact Binary V2790 Ori: Evidence for a Brown Dwarf Companion and a Solar-like Magnetic Activity Cycle
por: Wang, Si-Rui, et al.
Publicado: (2025)

Mutual Validation of Datasets for Analyzing Tilt Angles in Solar Active Regions
por: Qin, Lang, et al.
Publicado: (2025)

Solar Cycle 25 Dynamics from Observational and Statistical Parameters: Characterization of the Maximum Phase and Rotational Behaviour
por: Gutiérrez, Homer Dávila
Publicado: (2025)

An Overview of Solar Orbiter Observations of Interplanetary Shocks in Solar Cycle 25
por: Trotta, D., et al.
Publicado: (2024)

The occurrence of powerful flares stronger than X10 class in Solar Cycles
por: Tan, Baolin, et al.
Publicado: (2025)

Effects of Various Bipolar Approximations of Active Regions on Solar Surface Magnetic Field Simulations
por: Luo, Yukun, et al.
Publicado: (2026)

Resonances and Stellar Cycles: Observations and Modelling
por: Katsova, M. M., et al.
Publicado: (2025)

Simulation of Solar Surface Flux Transport Constrained by Magnetic Power Spectra. I. Flux Transport Parameter
por: Luo, Yukun, 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)

Observations of Successive CMEs and their Successive Type II Solar Radio Bursts in the Corona
por: Vasanth, V.
Publicado: (2025)

A Data-constrained Magnetohydrodynamic Simulation of Successive X-class Flares in Solar Active Region 13842. II. Dynamics of the Solar Eruption Associated with the X9.0 Solar Flare
por: Matsumoto, Keitarou, et al.
Publicado: (2025)

Heating Mechanisms and Radio Response from the Solar Chromosphere to Corona
por: Tan, Baolin, et al.
Publicado: (2025)

Solar Cycle Prediction Using TCN Deep Learning Model with One-Step Pattern
por: Zhao, Cui, et al.
Publicado: (2025)

High-Resolution Observation and Magnetic Modeling of a Solar Minifilament: the Formation, Eruption and Failing Mechanisms
por: Teng, Weilin, et al.
Publicado: (2024)

Hemispheric Distribution of Solar Active Regions During Solar Cycles 23-25
por: Liu, Yuxia, et al.
Publicado: (2025)

Generation and Life Cycle of Solar Spicules
por: Saleem, Hamid, et al.
Publicado: (2023)

Which Solar Latitude Follows the Sunspot Cycle Exactly?
por: Raju, K P
Publicado: (2025)

The Longest Duration SGRE Event in Solar Cycle 25
por: Gopalswamy, Nat, et al.
Publicado: (2025)

On the Constraints and Observational Manifestations of Failed Solar Eruptions in Toroidal Magnetic Cage
por: Guo, Jinhan, et al.
Publicado: (2026)

High-Resolution Observation of Solar Prominence Plumes Induced by Enhanced Spicular Activity
por: Wang, Wensi, et al.
Publicado: (2025)

Minimal Roles of Solar Subsurface Meridional Flow in the distributed-shear Babcock-Leighton Dynamo
por: Jiang, Jie, et al.
Publicado: (2025)

Mid-Cycle Observations of CR Boo and Estimation of the System's Parameters
por: Boneva, Daniela, et al.
Publicado: (2021)

Toward a live homogeneous database of solar active regions based on SOHO/MDI and SDO/HMI synoptic magnetograms.II.parameters for solar cycle variability
por: Wang, Ruihui, et al.
Publicado: (2024)

Probing Solar Wind Structures with Solar Energetic Particle Observations from Solar Orbiter
por: Chen, Xiaohang, et al.
Publicado: (2026)

Predicting the Timing of the the Solar Cycle 25 Polar Field Reversal
por: Jha, Bibhuti Kumar, et al.
Publicado: (2024)

The Sun's Non-Potential Corona over Solar Cycle 24
por: Yeates, Anthony R.
Publicado: (2024)

Investigating the IBEX Ribbon Structure a Solar Cycle Apart
por: Dayeh, Maher A., et al.
Publicado: (2023)

Stereoscopic Observations of Solar X-ray Sources Explained by a Data-Constrained Magnetohydrodynamic Simulation
por: Matsumoto, Keitarou, et al.
Publicado: (2026)

The Influence of Magnetic Complexity of Active Regions on Solar Wind Properties During Solar Cycles 23 and 24
por: Shi, Xinzheng, et al.
Publicado: (2025)

Study of Solar Energetic Particles: their Source Regions, Flares and CMEs during Solar Cycles 23-24
por: Kumar, Raj, et al.
Publicado: (2025)

Spectral and Imaging Observations of a C2.3 White-Light Flare from the Advanced Space-Based Solar Observatory (ASO-S) and the Chinese H$α$ Solar Explorer (CHASE)
por: Li, Qiao, et al.
Publicado: (2024)

Solar Cycle Variation of Axial Orientations and Favorable Locations of Eruptive MFRs
por: Xie, Hong, et al.
Publicado: (2025)

A 22-Year Cycle of the Network Topology for Solar Active Regions
por: Flández, Eduardo, et al.
Publicado: (2024)

On the Northward Shift of the Heliospheric Current Sheet at the End of Solar Cycle 24
por: Li, Huichao, et al.
Publicado: (2024)

The Split Janus-faced Sun: Magnetic Rhythm and Duality in the Solar Cycle
por: Chen, Weiqi, et al.
Publicado: (2026)