A data-driven MHD simulation of the 2011-02-15 coronal mass ejection from Active Region NOAA 11158
Fuente:
arXiv
Guardado en:
| Autores principales: | Fan, Yuhong, Kazachenko, Maria D., Afanasyev, Andrey N., Fisher, George H. |
|---|---|
| Formato: | Preprint |
| Publicado: |
2024
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
Ejemplares similares
When Magnetic Field Lines Stretch, Snap, and Expand: A New Look at Solar Flares with L-maps
por: Kazachenko, Maria D., et al.
Publicado: (2025)
por: Kazachenko, Maria D., et al.
Publicado: (2025)
Photospheric Pore Rotation Associated with a C-class Flare from Spectropolarimetric Observations with DKIST
por: Yadav, Rahul, et al.
Publicado: (2024)
por: Yadav, Rahul, et al.
Publicado: (2024)
Detecting coronal mass ejections with machine learning methods
por: Vida, K., et al.
Publicado: (2024)
por: Vida, K., et al.
Publicado: (2024)
Helical flows along coronal loops following the launch of a coronal mass ejection
por: Nedal, Mohamed, et al.
Publicado: (2025)
por: Nedal, Mohamed, et al.
Publicado: (2025)
Stellar flares, superflares and coronal mass ejections -- entering the Big data era
por: Vida, Krisztián, et al.
Publicado: (2024)
por: Vida, Krisztián, et al.
Publicado: (2024)
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)
por: Nechaeva, A. B., et al.
Publicado: (2025)
Data-driven Radiative Magnetohydrodynamics Simulations with the MURaM Code: the Emergence of Active Region 11158 and the X2.2 Flare
por: Chen, Feng
Publicado: (2025)
por: Chen, Feng
Publicado: (2025)
Freely propagating flanks of wide coronal-mass-ejection-driven shocks: Modelling and observational insights
por: Wijsen, N., et al.
Publicado: (2025)
por: Wijsen, N., et al.
Publicado: (2025)
Three-part structure of solar coronal mass ejection observed in low coronal signatures of Solar Orbiter
por: Podladchikova, Tatiana, et al.
Publicado: (2024)
por: Podladchikova, Tatiana, et al.
Publicado: (2024)
SIP-IFVM: An observation-based magnetohydrodynamic model of coronal mass ejection
por: Wang, Haopeng, et al.
Publicado: (2025)
por: Wang, Haopeng, et al.
Publicado: (2025)
Multiple shocks generated by the 2024 May 14 coronal mass ejection
por: Nedal, Mohamed, et al.
Publicado: (2026)
por: Nedal, Mohamed, et al.
Publicado: (2026)
Topological ignition of the stealth coronal mass ejections
por: Dumin, Yurii V., et al.
Publicado: (2025)
por: Dumin, Yurii V., 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)
por: Normo, S., et al.
Publicado: (2024)
Constraining the onset height of coronal mass ejection driven shocks using near-Sun observations in visible and radio wavelengths
por: Kathiravan, C., et al.
Publicado: (2026)
por: Kathiravan, C., et al.
Publicado: (2026)
Implications of the abundance of halo coronal mass ejections for the strength of solar cycle 25
por: Gopalswamy, Nat, et al.
Publicado: (2024)
por: Gopalswamy, Nat, et al.
Publicado: (2024)
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)
por: Cheng, Lei, et al.
Publicado: (2024)
Probing coronal mass ejections inclination effects with EUHFORIA
por: Martinić, Karmen, et al.
Publicado: (2024)
por: Martinić, Karmen, et al.
Publicado: (2024)
Parameter effects on the total intensity of H I Lyα line for a modelled coronal mass ejection and its driven shock
por: Ying, Beili, et al.
Publicado: (2024)
por: Ying, Beili, et al.
Publicado: (2024)
Modelling non-radially propagating coronal mass ejections and forecasting the time of their arrival at Earth
por: Valentino, Angelos, et al.
Publicado: (2024)
por: Valentino, Angelos, et al.
Publicado: (2024)
Why could a new-born active region produce coronal mass ejections?
por: Yang, Hanzhao, et al.
Publicado: (2024)
por: Yang, Hanzhao, 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)
por: Veronig, Astrid M., et al.
Publicado: (2025)
Signatures of coronal mass ejections in differential emission measure analysis of the Sun as a star
por: Michailidis, Angelos, et al.
Publicado: (2026)
por: Michailidis, Angelos, et al.
Publicado: (2026)
Relationship between prominence eruptions and coronal mass ejections during solar cycle 24
por: Devi, Pooja, et al.
Publicado: (2025)
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)
por: Strickert, K. Markus, et al.
Publicado: (2024)
Effects of background solar wind and drag force on the propagation of coronal mass ejection driven shock
por: Wu, Chin-Chun, et al.
Publicado: (2024)
por: Wu, Chin-Chun, et al.
Publicado: (2024)
A type II solar radio burst without a coronal mass ejection association
por: Kumari, Anshu, et al.
Publicado: (2025)
por: Kumari, Anshu, et al.
Publicado: (2025)
Predicting coronal mass ejection travel times using enhanced model-guided machine learning
por: Lampani, M., et al.
Publicado: (2025)
por: Lampani, M., et al.
Publicado: (2025)
Flux rope formation through flux cancellation of sheared coronal arcades in a 3D convectively-driven MHD simulation
por: Furuseth, Sondre Vik, et al.
Publicado: (2025)
por: Furuseth, Sondre Vik, et al.
Publicado: (2025)
Internal magnetic field structures observed by PSP/WISPR in a filament related coronal mass ejection
por: Cappello, G. M., et al.
Publicado: (2024)
por: Cappello, G. M., et al.
Publicado: (2024)
Is it possible to detect coronal mass ejections on solar-type stars through extreme-ultraviolet spectral observations?
por: Yang, Zihao, et al.
Publicado: (2024)
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)
por: Bhattacharjee, Debesh, et al.
Publicado: (2025)
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)
por: Xu, Yu, et al.
Publicado: (2025)
Experimental evidence for coronal mass ejection suppression in strong stellar magnetic fields
por: Chen, S. N., et al.
Publicado: (2026)
por: Chen, S. N., et al.
Publicado: (2026)
Assessment of the near-Sun magnetic field of the 10 March 2022 coronal mass ejection observed by Solar Orbiter
por: Koya, Shifana, et al.
Publicado: (2024)
por: Koya, Shifana, et al.
Publicado: (2024)
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)
por: Baratashvili, Tinatin, et al.
Publicado: (2025)
3D MHD simulations of coronal loops heated via magnetic braiding I. Continuous driving
por: Cozzo, Gabriele, et al.
Publicado: (2025)
por: Cozzo, Gabriele, et al.
Publicado: (2025)
SIP-IFVM: Efficient time-accurate magnetohydrodynamic model of the corona and coronal mass ejections
por: Wang, H. P., et al.
Publicado: (2024)
por: Wang, H. P., et al.
Publicado: (2024)
Evidence of energy conversion in weakly collisional plasma during an interplanetary coronal mass ejection
por: Dhamane, Omkar, et al.
Publicado: (2026)
por: Dhamane, Omkar, et al.
Publicado: (2026)
Various Features of the X-class White-light Flares in Super Active Region NOAA 13664
por: Li, Ying, et al.
Publicado: (2024)
por: Li, Ying, et al.
Publicado: (2024)
Magnetic interaction of stellar coronal mass ejections with close-in exoplanets: implication on planetary mass loss and Ly-$α$ transits
por: Hazra, Gopal, et al.
Publicado: (2024)
por: Hazra, Gopal, et al.
Publicado: (2024)
Ejemplares similares
-
When Magnetic Field Lines Stretch, Snap, and Expand: A New Look at Solar Flares with L-maps
por: Kazachenko, Maria D., et al.
Publicado: (2025) -
Photospheric Pore Rotation Associated with a C-class Flare from Spectropolarimetric Observations with DKIST
por: Yadav, Rahul, et al.
Publicado: (2024) -
Detecting coronal mass ejections with machine learning methods
por: Vida, K., et al.
Publicado: (2024) -
Helical flows along coronal loops following the launch of a coronal mass ejection
por: Nedal, Mohamed, et al.
Publicado: (2025) -
Stellar flares, superflares and coronal mass ejections -- entering the Big data era
por: Vida, Krisztián, et al.
Publicado: (2024)