Image de couverture de livre

Observing the evolution of the Sun's global coronal magnetic field over eight months

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Yang, Zihao, Tian, Hui, Tomczyk, Steven, Liu, Xianyu, Gibson, Sarah, Morton, Richard J., Downs, Cooper
Format:	Preprint
Publié:	2024
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

Measurements of the solar coronal magnetic field based on coronal seismology with propagating Alfvenic waves: forward modeling
par: Gao, Yuhang, et autres
Publié: (2024)

Mapping the Sun's coronal magnetic field using the Zeeman effect
par: Schad, Thomas A., et autres
Publié: (2024)

The fine-scale structure of polar coronal holes
par: Morton, Richard J., et autres
Publié: (2025)

High-frequency coronal Alfvénic waves observed with DKIST/Cryo-NIRSP
par: Morton, Richard J., et autres
Publié: (2025)

Assessment of the near-Sun magnetic field of the 10 March 2022 coronal mass ejection observed by Solar Orbiter
par: Koya, Shifana, et autres
Publié: (2024)

On the origins of coronal Alfvénic waves
par: Morton, R. J., et autres
Publié: (2025)

Coronal dimmings and what they tell us about solar and stellar coronal mass ejections
par: Veronig, Astrid M., et autres
Publié: (2025)

Unipolarity of the solar magnetic field in equatorial coronal holes
par: Katuwal, Khagendra, et autres
Publié: (2026)

Multi-episodes of remote brightenings driven by a coronal EUV jet on the Sun
par: Zhang, Chao, et autres
Publié: (2025)

Three types of solar coronal rain during magnetic reconnection between open and closed magnetic structures
par: Qiao, Fangfang, et autres
Publié: (2024)

The coronal power spectrum from MHD mode conversion above sunspots
par: Miriyala, Hemanthi, et autres
Publié: (2025)

Is it possible to detect coronal mass ejections on solar-type stars through extreme-ultraviolet spectral observations?
par: Yang, Zihao, et autres
Publié: (2024)

Asymmetry of the spectral lines of the coronal hole and quiet Sun in the transition region
par: Hosseini, Razieh, et autres
Publié: (2024)

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT
par: Wang, Haopeng, et autres
Publié: (2026)

Estimating the Poynting flux of Alfvénic waves in polar coronal holes across Solar Cycle 24
par: Morton, Richard J., et autres
Publié: (2025)

Stability of the coronal magnetic field around large confined and eruptive solar flares
par: Gupta, Manu, et autres
Publié: (2024)

Dynamics of the coronal magnetic field in the 2022-10-02 X-class flare
par: Fleishman, Gregory D., et autres
Publié: (2026)

Dependence of the intensity of the nonwave component of EUV waves on coronal magnetic field configuration
par: Li, Yuwei, et autres
Publié: (2025)

Quantifying how Surface Complexity Influences Properties of the Solar Corona and Solar Wind
par: Evans, Caroline L., et autres
Publié: (2025)

The first out-of-ecliptic observations of the polar magnetic field of the Sun
par: Calchetti, D., et autres
Publié: (2025)

A search for chemical stratification and magnetic fields in eight field blue horizontal-branch stars
par: Kafando, Issouf, et autres
Publié: (2025)

Failure of a solar filament eruption caused by magnetic reconnection with overlying coronal loops
par: Li, Leping, et autres
Publié: (2024)

Signatures of coronal mass ejections in differential emission measure analysis of the Sun as a star
par: Michailidis, Angelos, et autres
Publié: (2026)

Giant post-flare loops in active regions with extremely strong coronal magnetic fields
par: Alissandrakis, Costas E., et autres
Publié: (2024)

Three-dimensional mapping of coronal magnetic field and plasma parameters in a solar flare
par: Kaltman, Tatyana, et autres
Publié: (2026)

The Sun as an X-ray star V.: A new method to retrieve coronal filling factors
par: Joseph, Wilhelmina Maryann, et autres
Publié: (2025)

Temporal evolution of axially standing kink motions in solar coronal slabs: An eigenfunction expansion approach
par: Gao, Yuhong, et autres
Publié: (2024)

Nonlinear evolution of fluting oscillations in coronal flux tubes
par: Soler, Roberto, et autres
Publié: (2024)

On the magnetic field evolution of interplanetary coronal mass ejections from 0.07 to 5.4 au
par: Möstl, Christian, et autres
Publié: (2025)

Heating and cooling at a coronal magnetic null
par: Cargill, P. J., et autres
Publié: (2025)

SIP-IFVM: A time-evolving coronal model with an extended magnetic field decomposition strategy
par: Wang, Haopeng, et autres
Publié: (2025)

Nested active regions anchor the heliospheric current sheet and stall the reversal of the coronal magnetic field
par: Finley, Adam J.
Publié: (2024)

SynCOM: A tool for simulating coronal outflows
par: Filho, Valmir Moraes, et autres
Publié: (2024)

Understanding the complex morphology of a CME II: how pre-eruptive conditions shape CME evolution
par: Sahade, Abril, et autres
Publié: (2026)

Investigating explosive events in a 3D quiet-Sun model: Transition region and coronal response
par: Chen, Yajie, et autres
Publié: (2024)

Internal magnetic field structures observed by PSP/WISPR in a filament related coronal mass ejection
par: Cappello, G. M., et autres
Publié: (2024)

Oscillatory magnetic reconnection at a coronal bright point
par: Hong, Junchao, et autres
Publié: (2025)

Magnetic field dependence of bipolar magnetic region tilts on the Sun: Indication of tilt quenching
par: Jha, Bibhuti Kumar, et autres
Publié: (2019)

Generation and annihilation of three dimensional magnetic nulls in extrapolated solar coronal magnetic field: Data-based Implicit Large Eddy Simulation
par: Maurya, Yogesh Kumar, et autres
Publié: (2024)

Stereoscopic observations reveal coherent morphology and evolution of solar coronal loops
par: Ram, B., et autres
Publié: (2024)