:: Library Catalog

Imagen de Portada

Guardado en:

Detalles Bibliográficos
Autores principales:	Ni, Lei, Lin, Jun, Samanta, Tanmoy, Cheng, Guanchong, Wang, Yifu, Erdelyi, Robert
Formato:	Preprint
Publicado:	2026
Materias:	Solar and Stellar Astrophysics
Acceso en línea:	https://arxiv.org/abs/2602.19953
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

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

A magnetic reconnection model for the hot explosion with both ultraviolet and Hα wing emissions
por: Cheng, Guanchong, et al.
Publicado: (2024)

Numerical simulation of oscillatory magnetic reconnection modulated by solar convective motions
por: Wang, Yifu, et al.
Publicado: (2025)

Three dimensional magnetic reconnection mediated with plasmoids and the resulted multi-thermal emissions in the cool atmosphere of the Sun
por: Cheng, Guanchong, et al.
Publicado: (2025)

Evidence for Plasmoid-mediated Magnetic Reconnection during a Small-scale Flare in the Partially Ionized Low Solar Atmosphere
por: Cheng, Guanchong, et al.
Publicado: (2024)

The effect of plasma-$β$ on the heating mechanisms during magnetic reconnection in partially ionized low solar atmosphere
por: Zafar, Abdullah, et al.
Publicado: (2025)

Simulation of solar energetic particle events originated from coronal mass ejection shocks with a data-driven physics-based transport model
por: Cheng, Lei, et al.
Publicado: (2024)

Modelling the connection between propagating disturbances and solar spicules
por: Skirvin, Samuel, et al.
Publicado: (2024)

Three-dimensional kink modes in solar coronal slabs: group velocities and their implications for impulsively excited waves
por: Liu, Jing, et al.
Publicado: (2026)

Unipolarity of the solar magnetic field in equatorial coronal holes
por: Katuwal, Khagendra, et al.
Publicado: (2026)

A type II solar radio burst without a coronal mass ejection association
por: Kumari, Anshu, et al.
Publicado: (2025)

Helical flows along coronal loops following the launch of a coronal mass ejection
por: Nedal, Mohamed, et al.
Publicado: (2025)

The influence of different coronal hole geometries on simulations of coronal wave -- coronal hole interaction
por: Piantschitsch, I., et al.
Publicado: (2024)

Three-part structure of solar coronal mass ejection observed in low coronal signatures of Solar Orbiter
por: Podladchikova, Tatiana, et al.
Publicado: (2024)

Inferring photospheric horizontal flows from multiple observations with SUVEL models
por: Xie, Quan, et al.
Publicado: (2026)

On the possibility of using decayless kink oscillations of coronal loops to forecast powerful solar flares and coronal mass ejections
por: Nechaeva, A. B., et al.
Publicado: (2025)

Implications of the abundance of halo coronal mass ejections for the strength of solar cycle 25
por: Gopalswamy, Nat, et al.
Publicado: (2024)

Theoretical Studies on the Evolution of Solar Filaments in Response to New Emerging Flux
por: Chen, Yuhao, et al.
Publicado: (2024)

Spinning solar jets explained through the interplay between plasma sheets and vortex columns
por: Dey, Sahel, et al.
Publicado: (2024)

Coronal dimmings and what they tell us about solar and stellar coronal mass ejections
por: Veronig, Astrid M., et al.
Publicado: (2025)

Relationship between prominence eruptions and coronal mass ejections during solar cycle 24
por: Devi, Pooja, et al.
Publicado: (2025)

High-latitude coronal mass ejections on the young solar-like star AB Dor
por: Strickert, K. Markus, et al.
Publicado: (2024)

Simulations of coronal mass ejections on a young solar-type star and their detectability through coronal spectral observations
por: Xu, Yu, et al.
Publicado: (2025)

Probing the CME Core--Prominence Relation Using Inner Coronal Observations
por: Pradhan, Sunit Sundar, et al.
Publicado: (2026)

Is it possible to detect coronal mass ejections on solar-type stars through extreme-ultraviolet spectral observations?
por: Yang, Zihao, et al.
Publicado: (2024)

Proton heating estimates from near-Earth observations of coronal mass ejections in solar cycle 24
por: Bhattacharjee, Debesh, et al.
Publicado: (2025)

Investigating the propagation of small-scale flare energy in the lower and upper atmosphere of solar active region
por: Gupta, Girjesh, et al.
Publicado: (2026)

Challenges in identifying the coronal hole wind
por: Heidrich-Meisner, Verena, et al.
Publicado: (2025)

The fine-scale structure of polar coronal holes
por: Morton, Richard J., et al.
Publicado: (2025)

Measurements of the solar coronal magnetic field based on coronal seismology with propagating Alfvenic waves: forward modeling
por: Gao, Yuhang, et al.
Publicado: (2024)

Presence of solar inner F-corona and coronal heating
por: Qu, Z. Q., et al.
Publicado: (2025)

Long-lived coronal loops in solar active regions
por: Vasantharaju, N., et al.
Publicado: (2025)

Anomalous cross-field motions of solar coronal loops
por: Mandal, Sudip, et al.
Publicado: (2025)

Time-evolving coronal modelling of the solar maximum around the solar storms in May 2024 by COCONUT
por: Wang, Haopeng, et al.
Publicado: (2025)

Evolution of solar and stellar coronal abundances due to magnetic activity
por: Brooks, David H., et al.
Publicado: (2025)

Investigating the impact of the dynamic solar wind on the propagation of a coronal mass ejection with two models and multi-spacecraft measurements
por: Baratashvili, Tinatin, et al.
Publicado: (2025)

Estimating the lateral speed of a fast shock driven by a coronal mass ejection at the location of solar radio emissions
por: Normo, S., et al.
Publicado: (2024)

Detecting coronal mass ejections with machine learning methods
por: Vida, K., et al.
Publicado: (2024)

On the Origin of Coronal Picoflare Jets
por: Bura, Annu, et al.
Publicado: (2026)

Radiation magnetohydrodynamics modeling of an impulsively driven chromospheric jet in the solar atmosphere
por: González-Avilés, J. J.
Publicado: (2025)