Imagen de Portada

Finite Plasma Beta Three-dimensional Magnetic Field Extrapolation Based on MHD Relaxation Method

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Yamasaki, Daiki, Miyoshi, Takahiro, Inoue, Satoshi
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

Acceleration of Solar Eruptions via Enhanced Torus Instability Driven by Small-Scale Flux Emergence
por: Inoue, Satoshi, et al.
Publicado: (2025)

Observational Comparison Between Confined and Eruptive Flares: Magnetohydrodynamics Instability Parameters in a Similar Magnetic Configuration
por: Teraoka, Kouhei, et al.
Publicado: (2025)

Derivation and Application of a Scaling Between Hinode/SP and SDO/HMI Vector Magnetic Fields to Improve Magnetic Field Extrapolations
por: Beck, C., et al.
Publicado: (2024)

Radiative MHD Studies of Solar Spicules: Driving Mechanisms and the Role of Background Magnetic Field
por: Li, Jin, et al.
Publicado: (2026)

Adjusting the Potential Field Source Surface Height Based on MHD Simulations
por: Huang, Zhenguang, et al.
Publicado: (2024)

Study of Reconnection Dynamics and Plasma Relaxation in MHD simulation of a Solar Flare
por: Agarwal, Satyam, et al.
Publicado: (2024)

Nuclear Stellar Disk-like Nature in the Kinematics of SiO Maser Stars around Sagittarius A*
por: Tsuboi, Masato, et al.
Publicado: (2025)

Large Magnetic Flux Rope Formation in an X2.1 Flare observed on September 6, 2011
por: Roddanavar, Arpita, et al.
Publicado: (2025)

A New Multi-Constraint Potential Field Source Surface (PFSS) Extrapolation Model
por: Antonio, C., et al.
Publicado: (2026)

Multiple Extreme Ultraviolet Peaks Attributed to Three-dimensional Magnetic Reconnection in a Long-duration Solar Flare
por: Li, Shihan, et al.
Publicado: (2026)

Energetics and Emission in a Simulated Solar Flare Initialised by a Non-Force Free Magnetic Field
por: Bate, W., et al.
Publicado: (2026)

MHD Simulations of Strongly Magnetized HII Region Evolution: Evidence for Ionized Gas Filamentation
por: Crowe, Samuel, et al.
Publicado: (2026)

Driving mechanisms of solar active region geysers: The role of interacting magnetic flux
por: Monga, Aabha, et al.
Publicado: (2025)

Analytic Model and Magnetohydrodynamic Simulations of Three-dimensional Magnetic Switchbacks
por: Shi, Chen, et al.
Publicado: (2024)

A Tale of Three: Magnetic Fields along the Orion Integral-Shaped Filament as Revealed by JCMT BISTRO survey
por: Wu, Jintai, et al.
Publicado: (2024)

Formation of a Magnetic Flux Rope Prior to the Eruption: Insight from a Radiative MHD Simulation of Active Region Emergence
por: Wang, Can, et al.
Publicado: (2025)

Bidirectional Plasma Jets Driven by Magnetic Reconnection: Observations by GST and SDO
por: Liu, Yangyu, et al.
Publicado: (2026)

Prediction of Large Solar Flares Based on SHARP and HED Magnetic Field Parameters
por: Li, Xuebao, et al.
Publicado: (2024)

Diffusion Modeling of the Three-Dimensional Magnetic Field in the Sun's Corona
por: da Silva, Daniel E., et al.
Publicado: (2025)

Comparison of Polar Magnetic Fields Derived from MILOS and MERLIN Inversions with Hinode/SOT-SP Data
por: Kubo, Masahito, et al.
Publicado: (2025)

Effects of Grain Magnetic Properties and Grain Growth on Synthetic Dust Polarization of MHD Simulations in Protostellar Environments
por: Giang, Nguyen Chau, et al.
Publicado: (2023)

Quantitative Image-Based Validation Framework for Assessing Global Coronal Magnetic Field Models
por: Rura, Christopher E., et al.
Publicado: (2025)

A Data-constrained Magnetohydrodynamic Simulation of Successive X-class Flares in Solar Active Region 13842 I. Dynamics of the Solar Eruption Associated with the X7.1 Solar Flare
por: Matsumoto, Keitarou, et al.
Publicado: (2025)

Direct Imaging of a Prolonged Plasma/Current Sheet and Quasiperiodic Magnetic Reconnection on the Sun
por: Kumar, Pankaj, et al.
Publicado: (2024)

Three-dimensional velocity fields of the solar filament eruptions detected by CHASE
por: Qiu, Ye, et al.
Publicado: (2024)

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

Exploring the Origin and Dynamics of Solar Magnetic Fields
por: Hazra, Soumitra
Publicado: (2016)

MHD Modeling of the Molecular Filament Evolution
por: Sultanov, I. M., et al.
Publicado: (2024)

Poynting flux of MHD modes in magnetic solar vortex tubes
por: Skirvin, Samuel, et al.
Publicado: (2024)

Three-dimensional Reconstruction and Propagation of an Asymmetric Flux-rope Coronal Mass Ejection
por: Lamy, Philippe, et al.
Publicado: (2025)

Magnetic Fields in the Pillars of Creation
por: Sarkar, Adwitiya, et al.
Publicado: (2025)

Atmospheric Gravity Waves Modulated by the Magnetic Field Configuration
por: Vesa, Oana, et al.
Publicado: (2025)

Vortex Dynamics in Various Solar Magnetic Field Configurations
por: Kannan, Arjun, et al.
Publicado: (2024)

Confirming the Magnetic Field Detection at the Surface of $χ$ Cyg
por: Lavail, Alexis, et al.
Publicado: (2025)

Magnetic Field Evolution of the Solar Active Region 13664
por: Jarolim, Robert, et al.
Publicado: (2024)

On the Geometry of the Near-Core Magnetic Field in Massive Stars
por: Ratnasingam, Rathish P., et al.
Publicado: (2024)

Some Questions and Challenges in Measurements of Solar Magnetic Fields
por: Zhang, Hongqi, et al.
Publicado: (2025)

Basic Pattern of Three-dimensional Magnetic Reconnection within Strongly Turbulent Current Sheets
por: Wang, Yulei, et al.
Publicado: (2025)

Spectropolarimetric synthesis of forbidden lines in MHD models of coronal bright points
por: Ballester, Ernest Alsina, et al.
Publicado: (2025)

Observations of microwave emission from solar jets and comparison with MHD simulations
por: Alissandrakis, Costas E., et al.
Publicado: (2025)