SIP-IFVM: Efficient time-accurate magnetohydrodynamic model of the corona and coronal mass ejections
Fuente:
arXiv
Saved in:
| Main Authors: | Wang, H. P., Guo, J. H., Yang, L. P., Poedts, S., Zhang, F., Lani, A., Baratashvili, T., Linan, L., Lin, R., Guo, Y. |
|---|---|
| Format: | Preprint |
| Published: |
2024
|
| Subjects: | |
| Online Access: | |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
SIP-IFVM: An observation-based magnetohydrodynamic model of coronal mass ejection
by: Wang, Haopeng, et al.
Published: (2025)
by: Wang, Haopeng, et al.
Published: (2025)
Efficient magnetohydrodynamic modelling of the time-evolving corona by COCONUT
by: Wang, Haopeng, et al.
Published: (2024)
by: Wang, Haopeng, et al.
Published: (2024)
How coronal mass ejections are influenced by the morphology and toroidal flux of their source magnetic flux ropes?
by: Guo, J. H., et al.
Published: (2024)
by: Guo, J. H., et al.
Published: (2024)
The operationally ready full three-dimensional magnetohydrodynamic (3D MHD) model from the Sun to Earth: COCONUT+Icarus
by: Baratashvili, Tinatin, et al.
Published: (2024)
by: Baratashvili, Tinatin, et al.
Published: (2024)
CME propagation in the dynamically coupled space weather tool: COCONUT + EUHFORIA
by: Linan, L., et al.
Published: (2024)
by: Linan, L., et al.
Published: (2024)
SIP-IFVM: A time-evolving coronal model with an extended magnetic field decomposition strategy
by: Wang, Haopeng, et al.
Published: (2025)
by: Wang, Haopeng, et al.
Published: (2025)
The effect of AMR and grid stretching on the magnetized CME model in Icarus
by: Baratashvili, Tinatin, et al.
Published: (2024)
by: Baratashvili, Tinatin, et al.
Published: (2024)
Topological ignition of the stealth coronal mass ejections
by: Dumin, Yurii V., et al.
Published: (2025)
by: Dumin, Yurii V., et al.
Published: (2025)
Probing coronal mass ejections inclination effects with EUHFORIA
by: Martinić, Karmen, et al.
Published: (2024)
by: Martinić, Karmen, et al.
Published: (2024)
Freely propagating flanks of wide coronal-mass-ejection-driven shocks: Modelling and observational insights
by: Wijsen, N., et al.
Published: (2025)
by: Wijsen, N., et al.
Published: (2025)
Toroidal modified Miller-Turner CME model in EUHFORIA: II. Validation and comparison with flux rope and spheromak
by: Maharana, Anwesha, et al.
Published: (2024)
by: Maharana, Anwesha, et al.
Published: (2024)
Can metric radio bursts be used as a diagnostics tool for interplanetary coronal mass ejections?
by: Kandekar, J., et al.
Published: (2025)
by: Kandekar, J., et al.
Published: (2025)
Effects of background solar wind and drag force on the propagation of coronal mass ejection driven shock
by: Wu, Chin-Chun, et al.
Published: (2024)
by: Wu, Chin-Chun, et al.
Published: (2024)
Evolution of interacting coronal mass ejections driving the great geomagnetic storm on 10 May 2024
by: Khuntia, Soumyaranjan, et al.
Published: (2025)
by: Khuntia, Soumyaranjan, et al.
Published: (2025)
Investigating the impact of the dynamic solar wind on the propagation of a coronal mass ejection with two models and multi-spacecraft measurements
by: Baratashvili, Tinatin, et al.
Published: (2025)
by: Baratashvili, Tinatin, et al.
Published: (2025)
Multi spacecraft study with the Icarus model: Modelling the propagation of CMEs to Mercury and Earth
by: Baratashvili, Tinatin, et al.
Published: (2024)
by: Baratashvili, Tinatin, et al.
Published: (2024)
On the magnetic field evolution of interplanetary coronal mass ejections from 0.07 to 5.4 au
by: Möstl, Christian, et al.
Published: (2025)
by: Möstl, Christian, et al.
Published: (2025)
Energetic particle acceleration and transport with the novel Icarus$+$PARADISE model
by: Husidic, Edin, et al.
Published: (2024)
by: Husidic, Edin, et al.
Published: (2024)
A coronal mass ejection encountered by four spacecraft within 1 au from the Sun: Ensemble modelling of propagation and magnetic structure
by: Palmerio, Erika, et al.
Published: (2024)
by: Palmerio, Erika, et al.
Published: (2024)
Evolution of coronal mass ejections with and without sheaths from the inner to the outer heliosphere -- statistical investigation for 1975-2022
by: Larrodera, C., et al.
Published: (2024)
by: Larrodera, C., et al.
Published: (2024)
Understanding the effects of spacecraft trajectories through solar coronal mass ejection flux ropes using 3DCOREweb
by: Rüdisser, Hannah Theresa, et al.
Published: (2024)
by: Rüdisser, Hannah Theresa, et al.
Published: (2024)
Validity of using Elsässer variables to study the interaction of compressible solar wind fluctuations with a coronal mass ejection
by: Sishtla, Chaitanya Prasad, et al.
Published: (2024)
by: Sishtla, Chaitanya Prasad, et al.
Published: (2024)
Diagnostics of the solar coronal plasmas by magnetohydrodynamic waves: Magnetohydrodynamic seismology
by: Nakariakov, Valery M., et al.
Published: (2024)
by: Nakariakov, Valery M., et al.
Published: (2024)
Magnetic interaction analysis of multiple interplanetary coronal mass ejections leading to a historic geomagnetic storm in May 2024
by: Pal, Sanchita, et al.
Published: (2025)
by: Pal, Sanchita, et al.
Published: (2025)
Modelling gyrosynchrotron emission from coronal energetic electrons in a CME flux rope
by: Husidic, Edin, et al.
Published: (2025)
by: Husidic, Edin, et al.
Published: (2025)
Data-driven Magnetohydrodynamic Simulation of the Initiation of a Coronal Mass Ejection with Multiple Stages
by: Guo, J. H., et al.
Published: (2026)
by: Guo, J. H., et al.
Published: (2026)
Recent advances in solar data-driven MHD simulations of the formation and evolution of CME flux ropes
by: Schmieder, Brigitte, et al.
Published: (2024)
by: Schmieder, Brigitte, et al.
Published: (2024)
Cross-Field Diffusion Effects on Particle Transport in a Solar Coronal Flux Rope
by: Husidic, Edin, et al.
Published: (2024)
by: Husidic, Edin, et al.
Published: (2024)
HelioFill: Diffusion-Based Model for EUV Reconstruction of the Solar Farside
by: Ameur, Firas Ben, et al.
Published: (2025)
by: Ameur, Firas Ben, et al.
Published: (2025)
Flare energetics, CME launch and heliospheric propagation for the May 2024 events, as derived from ensemble MHD modelling
by: Schmieder, Brigitte, et al.
Published: (2025)
by: Schmieder, Brigitte, et al.
Published: (2025)
Magnetic connectivity from the Sun to the Earth with MHD models I. Impact of the magnetic modelling for connectivity validation
by: Kennis, Silke, et al.
Published: (2024)
by: Kennis, Silke, et al.
Published: (2024)
Total solar eclipse 2024 modelling with COCONUT
by: Baratashvili, Tinatin, et al.
Published: (2025)
by: Baratashvili, Tinatin, et al.
Published: (2025)
Time-evolving coronal modelling of the solar maximum around the solar storms in May 2024 by COCONUT
by: Wang, Haopeng, et al.
Published: (2025)
by: Wang, Haopeng, et al.
Published: (2025)
Density-gradient-driven drift waves in the solar corona
by: Brchnelova, Michaela, et al.
Published: (2024)
by: Brchnelova, Michaela, et al.
Published: (2024)
Imaging spectroscopy reveals spike-like repeating radio burst pairs in the solar corona
by: Ma, Suli, et al.
Published: (2026)
by: Ma, Suli, et al.
Published: (2026)
Coronal mass ejection arrival forecasting with the drag-based assimilation of satellite observations
by: Abu-Shaar, Zaina, et al.
Published: (2025)
by: Abu-Shaar, Zaina, et al.
Published: (2025)
COCONUT: A coronal model with an energy decomposition strategy
by: Wang, Haopeng, et al.
Published: (2025)
by: Wang, Haopeng, et al.
Published: (2025)
Data-constrained 3D MHD Simulation of a Spiral Jet Caused by an Unstable Flux Rope Embedded in Fan-spine Configuration
by: Li, Z. F., et al.
Published: (2025)
by: Li, Z. F., et al.
Published: (2025)
Icarus 3.0: Dynamic Heliosphere Modelling
by: Baratashvili, Tinatin, et al.
Published: (2025)
by: Baratashvili, Tinatin, et al.
Published: (2025)
Constraining the inner boundaries of COCONUT through plasma \b{eta} and Alfvén speed
by: Brchnelova, Michaela, et al.
Published: (2024)
by: Brchnelova, Michaela, et al.
Published: (2024)
Similar Items
-
SIP-IFVM: An observation-based magnetohydrodynamic model of coronal mass ejection
by: Wang, Haopeng, et al.
Published: (2025) -
Efficient magnetohydrodynamic modelling of the time-evolving corona by COCONUT
by: Wang, Haopeng, et al.
Published: (2024) -
How coronal mass ejections are influenced by the morphology and toroidal flux of their source magnetic flux ropes?
by: Guo, J. H., et al.
Published: (2024) -
The operationally ready full three-dimensional magnetohydrodynamic (3D MHD) model from the Sun to Earth: COCONUT+Icarus
by: Baratashvili, Tinatin, et al.
Published: (2024) -
CME propagation in the dynamically coupled space weather tool: COCONUT + EUHFORIA
by: Linan, L., et al.
Published: (2024)