Image de couverture de livre

The Kinematical Behavior of Solar Eruptive Filaments Affected by the Poloidal Magnetic Field

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Qiu, Ye, Guo, Yang, Ding, Mingde, Li, Chuan, Kong, Linggao, Li, Zhen
Format:	Preprint
Publié:	2025
Sujets:	Solar and Stellar Astrophysics
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

Documents similaires

Three-dimensional velocity fields of the solar filament eruptions detected by CHASE
par: Qiu, Ye, et autres
Publié: (2024)

Rotation of a Solar Jet Driven by Plasma Flow along Helical Magnetic Fields in an Active Region
par: Huang, Lei, et autres
Publié: (2026)

Partial Null Point Reconnection of an Eruptive Filament
par: Devi, Pooja, et autres
Publié: (2025)

Deflection of a Filament Eruption with Three Parallel Flare Ribbons via Reconnection at an X-Point
par: Zhang, Xiaomeng, et autres
Publié: (2026)

Initiation Route of Coronal Mass Ejections: II. The Role of Filament Mass
par: Xing, Chen, et autres
Publié: (2025)

Influence of Cross-sectional Expansion on Coronal Emissions from a Radiatively Cooling Solar Flare Loop
par: Dai, Yu, et autres
Publié: (2026)

Multiwavelength Observations of the Precursors Before the Eruptive X4.9 Limb Solar Flare on 25 February, 2014: Current Sheet, Eruptive Filament, Flare and Eruption Onset in the Frame of the Tether-Cutting Magnetic Reconnection Scenario
par: N., Sharykin I., et autres
Publié: (2025)

Multiple Extreme Ultraviolet Peaks Attributed to Three-dimensional Magnetic Reconnection in a Long-duration Solar Flare
par: Li, Shihan, et autres
Publié: (2026)

Enhanced Peak and Extended Cooling of the Extreme-ultraviolet Late Phase in a Confined Solar Flare
par: Li, Shihan, et autres
Publié: (2024)

Particle Acceleration and Transport in the Large-scale Current Sheet under an Erupting Magnetic Flux Rope
par: Wu, Hao, et autres
Publié: (2025)

The Non-Eruptive Reconfiguration of a Quiescent Filament After a Nearby Active Region Emergence
par: McKevitt, James, et autres
Publié: (2026)

Investigation on the Predictive Potentiality of Photospheric Magnetic Parameters for Distinguishing Confined from Eruptive Solar Flares
par: Pan, Jinhui, et autres
Publié: (2025)

Dynamics of Reconnection Nanojets in Eruptive and Confined Solar Flares
par: Bura, Annu, et autres
Publié: (2025)

Polar Filaments Capture High Latitude Solar Poloidal Field Interactions and can Foretell the Future Sunspot Cycle Amplitude before Polar Field Precursors
par: Routh, Srinjana, et autres
Publié: (2025)

Analysis of Lyman-beta and Lyman-gamma Lines in a Pre-Eruptive and Eruptive Prominence with Solar Orbiter SPICE Observations
par: Zhang, Yong, et autres
Publié: (2026)

Simple Model for Temporal Variations of H$α$ Spectrum by an Eruptive Filament from a Superflare on a Solar-type Star
par: Ikuta, Kai, et autres
Publié: (2024)

Filament Mass Losses Forced by Magnetic Reconnection in the Solar Corona
par: Johnston, Craig D., et autres
Publié: (2025)

Minifilament Eruptions as the Last Straw to Break the Equilibrium of a Giant Solar Filament
par: Chen, Hechao, et autres
Publié: (2025)

Elongation of a Solar Filament and its Three-Dimensional Numerical Reconstruction for Magnetic Structures
par: Karki, Garima, et autres
Publié: (2026)

Solar Cycle Variation of Axial Orientations and Favorable Locations of Eruptive MFRs
par: Xie, Hong, et autres
Publié: (2025)

Sympathetic Eruption of Two Filaments and Associated Solar Coronal Jet
par: Yang, Jiayan, et autres
Publié: (2025)

Solar Filament Physiognomy: Inferring Magnetic Quantities from Imaging Observations
par: Chen, P. F.
Publié: (2025)

Magnetic Reconnection between a Solar Jet and a Filament Channel
par: Karki, Garima, et autres
Publié: (2024)

How Reconnection-Unfavored Magnetic Flux Emergence Suppresses Solar Filament Eruptions
par: Zhou, Chengrui, et autres
Publié: (2025)

Two-sided Loop Solar Jet Driven by the Eruption of a Small Filament in a Big Filament Channel
par: Yang, Jiayan, et autres
Publié: (2024)

The Hourglass-shaped Magnetic Fields and Dust Filaments in the HH 211 Protostellar Envelope
par: Choi, Youngwoo, et autres
Publié: (2025)

Prediction of Large Solar Flares Based on SHARP and HED Magnetic Field Parameters
par: Li, Xuebao, et autres
Publié: (2024)

Developing an Automated Detection, Tracking and Analysis Method for Solar Filaments Observed by CHASE via Machine Learning
par: Zheng, Z., et autres
Publié: (2024)

Can We Distinguish the Source Region Location of Filament/Prominence Eruptions from the Sun-as-a-star H$α$ Spectrum?
par: Zhang, Junyi, et autres
Publié: (2026)

Segmentation and Tracking of Eruptive Solar Phenomena with Convolutional Neural Networks
par: Stepanyuk, Oleg, et autres
Publié: (2025)

Basic Pattern of Three-dimensional Magnetic Reconnection within Strongly Turbulent Current Sheets
par: Wang, Yulei, et autres
Publié: (2025)

Survey of Magnetic Field Parameters Associated With Large Solar Flares
par: Li, Ting, et autres
Publié: (2024)

Theoretical Studies on the Evolution of Solar Filaments in Response to New Emerging Flux
par: Chen, Yuhao, et autres
Publié: (2024)

Microwave Imaging Spectroscopy Diagnosis of the Slow-rise Precursor of a Major Solar Eruption
par: Kou, Yuankun, et autres
Publié: (2025)

Observational Study of Recurrent Jets: Evolution of Magnetic Flux, Current, and Helicity
par: Zhou, Chang, et autres
Publié: (2025)

Data-constrained Magnetohydrodynamic Simulation of a Filament Eruption in a Decaying Active Region 13079 on a Global Scale
par: Li, Yihua, et autres
Publié: (2025)

Do Planets Affect the Behavior of the Long-term Solar Activity?
par: Katsova, M. M., et autres
Publié: (2025)

Long-Duration Nonthermal Motions in the Supra-Arcade and Loop-Top Region During an Eruptive Solar Flare
par: Gou, Tingyu, et autres
Publié: (2025)

Falling Threads During Solar Filament Eruptions
par: Wu, Yidian, et autres
Publié: (2025)

The Observations of Magnetic Reconnection During the Interaction Process of Two Active Region Filaments
par: Wu, Zongyin, et autres
Publié: (2025)