Imagen de Portada

Cosmic Ray Inter-Station Correlation Variations as Precursors of Geomagnetic Storms: A Statistical Study and Multi-Parameter Early Warning Framework

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Li, Haoyang, Ge, Zongyuan, Wang, Zhaoming
Formato:	Preprint
Publicado:	2026
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

Cosmic-Ray-Constrained LSTM Model for Geomagnetic Storm Prediction
por: Ge, Zongyuan, et al.
Publicado: (2025)

Multi-Energy Proton Events and Geomagnetic Storms in Solar Cycles 23 and 24
por: Miteva, Rositsa, et al.
Publicado: (2025)

A Major Geomagnetic Storm in 2024 October Linked to Sympathetic CME--Prominence Eruptions
por: Wang, Rui, et al.
Publicado: (2026)

Extreme Geomagnetic Storm on Early Earth Induced by Corotating Interaction Regions from the Young Sun
por: Sur, Dibyendu, et al.
Publicado: (2025)

Regression to the Mean of Extreme Geomagnetic Storms
por: Sivadas, Nithin, et al.
Publicado: (2022)

Geomagnetic Storms and Satellite Orbital Decay
por: Baruah, Yoshita
Publicado: (2025)

Intense Geomagnetic Storms during Solar Cycles 23-25
por: Gopalswamy, N., et al.
Publicado: (2024)

The Instantaneous Response of Geomagnetic Field, near-Earth IMF and Cosmic-Ray Intensity to Solar Flares
por: Takalo, Jouni J.
Publicado: (2024)

Geomagnetic Storm Impacts On The Ionosphere Over Türkiye During Solar Cycle 25: Focusing On The May 2024 Storm
por: Eraydın, Ege, et al.
Publicado: (2026)

Distribution and Recovery Phase of Geomagnetic Storms During Solar Cycles 23 and 24
por: Mishra, Wageesh, et al.
Publicado: (2024)

The Solar and Geomagnetic Storms in May 2024: A Flash Data Report
por: Hayakawa, Hisashi, et al.
Publicado: (2024)

Investigating Ionospheric TEC Variations in Solar and Geomagnetic Influences Across Solar Activity Phases
por: Hassan, Ziyadat, et al.
Publicado: (2026)

A Pileup of Coronal Mass Ejections Produced the Largest Geomagnetic Storm in Two Decades
por: Liu, Ying D., et al.
Publicado: (2024)

The Solar Origin of an Intense Geomagnetic Storm on 2023 December 1st: Successive Slipping and Eruption of Multiple Magnetic Flux Ropes
por: Sun, Zheng, et al.
Publicado: (2024)

Forbush Decreases during strong Geomagnetic Storms: Time Delays, Rigidity Effects, and ICME-Driven Modulation
por: Ahmed, O., et al.
Publicado: (2025)

Effects of Geomagnetic Cutoff Rigidity Variations during Forbush Decreases
por: Zhao, Pengwei, et al.
Publicado: (2026)

Deconstructing the Properties of Solar Super Active Region 13664 in the Context of the Historic Geomagnetic Storm of 2024 May 10-11
por: Jaswal, Priyansh, et al.
Publicado: (2024)

A Multi-Diagnostic Observational Framework for Magnetosonic Solitary Waves During Geomagnetic Storms in Solar Cycles 24 and 25 using Cluster II Mission
por: Khusroo, Murchana, et al.
Publicado: (2026)

How the CME on 21 April 2023 Triggered the First Severe Geomagnetic Storm of Solar Cycle 25
por: Paouris, Evangelos, et al.
Publicado: (2025)

The April 2023 SYM-H = -233 nT Geomagnetic Storm: A Classical Event
por: Hajra, Rajkumar, et al.
Publicado: (2024)

Temporal Correlation between Positive-Charged Cosmic Ray Flux and Solar Polar Field Variation: Insights from Delayed Modulation Analysis
por: Gong, Shaokun, et al.
Publicado: (2024)

A Statistical Analysis of Magnetic Parameters in Solar Source Regions of Halo-CMEs with and without SEP events
por: Duan, Xuchun, et al.
Publicado: (2025)

The ALMA Survey of 70 $μ$m Dark High-mass Clumps in Early Stages (ASHES). XI. Statistical Study of Early Fragmentation
por: Morii, Kaho, et al.
Publicado: (2024)

Correlating Intrinsic Stellar Parameters with Mg II Self-Reversal Depths
por: Taylor, Anna, et al.
Publicado: (2024)

Estimating the Atmospheric Parameters of Early-type Stars from the Chinese Space Station Telescope (CSST) Slitless Spectra Survey
por: Rao, JiaRui, et al.
Publicado: (2024)

Photometric and Spectroscopic Studies of Two Early-Type Eclipsing Binaries
por: Ye, Peng-Fei, et al.
Publicado: (2025)

Dynamics of Subsurface Flows in Solar Active Regions During the May 2024 Storm
por: Lekshmi, B, et al.
Publicado: (2025)

Pitch-Angle Scattering of Cosmic Rays: Confronting Theory with Observations
por: Yan, Huirong, et al.
Publicado: (2026)

Continuum And Line Emission From Accretion Shocks at T Tauri Stars I. Correlations With Shock Parameters
por: Kwan, John
Publicado: (2024)

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

Frequency-time-resolved Imaging Spectroscopy of Fine Structures in a Solar Radio Noise Storm
por: Clarkson, Daniel L., et al.
Publicado: (2026)

Observation and Modeling of Small Spatial Structures of Solar Radio Noise Storms using the uGMRT
por: Mondal, Surajit, et al.
Publicado: (2025)

Formation and Early Evolution of Protoplanetary Disks under Nonuniform Cosmic-Ray Ionization
por: Nishio, Erika, et al.
Publicado: (2025)

Modeling the Effect of the Heliospheric Magnetic Field on Cosmic Ray Muon Shadows
por: Collaboration, MINOS+, et al.
Publicado: (2026)

Stellar Parameters and Orbital Period Estimates for Composite-Spectrum sdB+MS Binaries from LAMOST
por: Li, Jiangdan, et al.
Publicado: (2026)

Improving Solar Flare Nowcasting with the Hot Onset Precursor Event (HOPE) Technique
por: Telikicherla, Anant, et al.
Publicado: (2025)

Statistical Study of Balmer Continuum Enhancement in Solar Flares
por: Sharma, Pranjali, et al.
Publicado: (2026)

Variations of the Ca II K Line Profile Parameters with Solar Latitude and Time Observed from Kodaikanal Solar Observatory
por: Srinivasa, Apoorva, et al.
Publicado: (2025)

Microwave Imaging Spectroscopy Diagnosis of the Slow-rise Precursor of a Major Solar Eruption
por: Kou, Yuankun, et al.
Publicado: (2025)

A Cosmic Ray Acceleration Mechanism Based on Background Flow Velocity Inhomogeneities Yielding Power-Law Spectra
por: Wang, J. -F., et al.
Publicado: (2025)