Imagen de Portada

Complexity of emerging magnetic flux during lifetime of solar ephemeral regions

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Yang, Hanlin, Jin, Chunlan, Wang, Zifan, Wang, Jingxiu
Formato:	Preprint
Publicado:	2024
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

Atmospheric Heating Events Associated with Fine-scale Flux Emergence in Ephemeral Regions
por: Yang, Hanlin, et al.
Publicado: (2025)

Variations of the vector magnetic structures in the solar polar regions observed by Hinode
por: Yang, Shuhong, et al.
Publicado: (2025)

Meridional flow in the solar polar caps revealed by magnetic field observation and simulation
por: Yang, Shuhong, et al.
Publicado: (2024)

Long-term variation of the solar polar magnetic fields at different latitudes
por: Yang, Shuhong, et al.
Publicado: (2024)

Estimation of gravitational wave from solar emerging magnetic flux tube
por: Guan, Siqi, et al.
Publicado: (2025)

A statistical study of magnetic flux emergence in solar active regions prior to strongest flares
por: Kutsenko, Alexander S., et al.
Publicado: (2021)

The rotation-magnetism relationship in solar-type stars. Constraining magnetic flux emergence rates
por: Isik, Emre, et al.
Publicado: (2025)

Low-latitude magnetic flux emergence on rapidly rotating solar-type stars
por: Işık, Emre, et al.
Publicado: (2024)

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

High flow speeds and transition-region like temperatures in the solar chromosphere during flux emergence
por: Leenaarts, J., et al.
Publicado: (2025)

Small-scale magnetic flux emergence preceding a chain of energetic solar atmospheric events
por: Nóbrega-Siverio, D., et al.
Publicado: (2024)

Hemispheric analysis of the magnetic flux in regular and irregular solar active regions
por: Zhukova, A.
Publicado: (2024)

Response of the solar atmosphere to flux emergence: With emergence-driven prominence formation
por: Li, Xiaohong, et al.
Publicado: (2025)

Statistical analysis of the total magnetic flux decay rate in solar active regions
por: Plotnikov, Andrei A., et al.
Publicado: (2023)

The nature of elongated granulations and stretched dark lanes in a newly emerging flux region
por: Wang, Jincheng, et al.
Publicado: (2024)

The role of nonlinear toroidal flux loss due to flux emergence in the long-term evolution of the solar cycle
por: Biswas, Akash
Publicado: (2024)

The role of photospheric magnetic flux diffusion in initiation of solar eruptions
por: Bian, Xinkai, et al.
Publicado: (2025)

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT
por: Wang, Haopeng, et al.
Publicado: (2026)

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

Large ephemeral regions and their tilt angles
por: Gupta, Rambahadur, et al.
Publicado: (2026)

Solar magnetic flux rope eruptions caused by inverse flux feeding processes
por: Zhang, Quanhao, et al.
Publicado: (2025)

Magnetograms underestimate even unipolar magnetic flux nearly everywhere on the solar disk
por: Sinjan, Jonas, et al.
Publicado: (2024)

Chromosphere of the quiet sun: II. Atmospheric response to small-scale magnetic flux emergence
por: Noraz, Quentin, et al.
Publicado: (2026)

A flux-independent increase in outflows prior to the emergence of active regions on the Sun
por: Schunker, Hannah, et al.
Publicado: (2024)

Magnetic helicity evolution during active region emergence and subsequent flare productivity
por: Sun, Zheng, et al.
Publicado: (2024)

Spatial extent of the magnetic influence of an active region on the solar atmosphere
por: Mann, Gottfried, et al.
Publicado: (2025)

Variation of the sunspot area during the rising and declining phases of the solar cycle supports the toroidal flux loss due to flux emergence
por: Karak, Bidya Binay, et al.
Publicado: (2026)

Magnetic helicity and energy budgets of jet events from an emerging solar active region
por: Nindos, A., et al.
Publicado: (2024)

Magnetic evolution of active regions: formation and eruption of magnetic flux ropes
por: Vemareddy, P.
Publicado: (2024)

Average solar active region: I. Intensities, velocities, and the photospheric magnetic field
por: Švanda, M., et al.
Publicado: (2025)

Time variations of the mean magnetic flux in active regions of different magneto-morphological classes
por: Zhukova, Anastasiya, et al.
Publicado: (2026)

Energy and helicity evolution in a flux emergence simulation
por: Moraitis, K., et al.
Publicado: (2024)

Estimation of the lifetime of slow-decaying unipolar active regions in the framework of the turbulent erosion model
por: Plotnikov, Andrei, et al.
Publicado: (2024)

Magnetic flux cancellation in a flux-emergence magnetohydrodynamics simulation of coronal hole eruptions and jets
por: Patsourakos, Spiros, et al.
Publicado: (2025)

The evolution of chromospheric quiet-sun bright points during their lifetime
por: Humphries, Llŷr, et al.
Publicado: (2025)

Spatial resolution effects on the solar open flux estimates
por: Milic, Ivan, et al.
Publicado: (2024)

Recurrent eruptions from the emergence of a toroidal flux tube
por: Zhuleku, J., et al.
Publicado: (2025)

Ultra-fast simulations of the solar dipole and open flux
por: Tähtinen, Ismo, et al.
Publicado: (2026)

Magnetic field and radial velocity fluxes at the initial stages of the evolution of solar active regions based on measurements at the photospheric level
por: Sadykov, Aidar M., et al.
Publicado: (2024)

Global impact of emerging internetwork fields on the low solar atmosphere
por: Gošić, Milan, et al.
Publicado: (2022)