Cover Image

Total solar eclipse 2024 modelling with COCONUT

Fuente: arXiv

Saved in:

Bibliographic Details
Main Authors:	Baratashvili, Tinatin, Wang, Haopeng, Sorokina, Daria, Lani, Andrea, Poedts, Stefaan
Format:	Preprint
Published:	2025
Subjects:	Solar and Stellar Astrophysics
Online Access:	Acceder al recurso
Tags:	Add Tag No Tags, Be the first to tag this record!

Similar Items

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

The operationally ready full three-dimensional magnetohydrodynamic (3D MHD) model from the Sun to Earth: COCONUT+Icarus
by: Baratashvili, Tinatin, et al.
Published: (2024)

Efficient magnetohydrodynamic modelling of the time-evolving corona by COCONUT
by: Wang, Haopeng, et al.
Published: (2024)

The effect of AMR and grid stretching on the magnetized CME model in Icarus
by: Baratashvili, Tinatin, et al.
Published: (2024)

COCONUT: A coronal model with an energy decomposition strategy
by: Wang, Haopeng, et al.
Published: (2025)

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

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)

CME propagation in the dynamically coupled space weather tool: COCONUT + EUHFORIA
by: Linan, L., et al.
Published: (2024)

Multi spacecraft study with the Icarus model: Modelling the propagation of CMEs to Mercury and Earth
by: Baratashvili, Tinatin, et al.
Published: (2024)

Energetic particle acceleration and transport with the novel Icarus$+$PARADISE model
by: Husidic, Edin, et al.
Published: (2024)

COCONUT: Toward practical time-evolving Sun-to-Earth magnetohydrodynamic modeling
by: Wang, Haopeng, et al.
Published: (2026)

Constraining the inner boundaries of COCONUT through plasma \b{eta} and Alfvén speed
by: Brchnelova, Michaela, et al.
Published: (2024)

SIP-IFVM: An observation-based magnetohydrodynamic model of coronal mass ejection
by: Wang, Haopeng, et al.
Published: (2025)

Icarus 3.0: Dynamic Heliosphere Modelling
by: Baratashvili, Tinatin, et al.
Published: (2025)

Comprehensive MHD modelling of ten successive CMEs driving a historic geomagnetic storm -- The 2024 Mothers Day event
by: Soni, Shirsh Lata, et al.
Published: (2026)

SIP-IFVM: A time-evolving coronal model with an extended magnetic field decomposition strategy
by: Wang, Haopeng, et al.
Published: (2025)

Recent advances in solar data-driven MHD simulations of the formation and evolution of CME flux ropes
by: Schmieder, Brigitte, et al.
Published: (2024)

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)

Kinetic-based macro-modeling of the solar wind at large heliocentric distances: Kappa electrons at the exobase
by: Vinogradov, Alexander, et al.
Published: (2026)

HelioFill: Diffusion-Based Model for EUV Reconstruction of the Solar Farside
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)

SIP-IFVM: Efficient time-accurate magnetohydrodynamic model of the corona and coronal mass ejections
by: Wang, H. P., et al.
Published: (2024)

Density-gradient-driven drift waves in the solar corona
by: Brchnelova, Michaela, et al.
Published: (2024)

Toroidal modified Miller-Turner CME model in EUHFORIA: II. Validation and comparison with flux rope and spheromak
by: Maharana, Anwesha, et al.
Published: (2024)

Cannibals in PARADISE: The effect of merging interplanetary shocks on solar energetic particle events
by: Niemela, Antonio, et al.
Published: (2024)

Rotation of flux ropes in the low corona
by: Schmieder, Brigitte, et al.
Published: (2025)

Elongation of a Solar Filament and its Three-Dimensional Numerical Reconstruction for Magnetic Structures
by: Karki, Garima, et al.
Published: (2026)

Employing the coupled EUHFORIA-OpenGGCM model to predict CME geoeffectiveness
by: Maharana, Anwesha, 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)

Cool matter distribution in inner solar corona from 2023 total solar eclipse observation
by: Qu, Z. Q., et al.
Published: (2024)

Absolute dimensions of solar-type eclipsing binaries. NY Hya: A test for magnetic stellar evolution models
by: Hinse, T. C., et al.
Published: (2024)

Expanding CGL: The CGL double-adiabatic approximation in the Expanding Solar Wind
by: Echeverría-Veas, Sebastián, et al.
Published: (2024)

Cross-Field Diffusion Effects on Particle Transport in a Solar Coronal Flux Rope
by: Husidic, Edin, et al.
Published: (2024)

The present and the future of modeling eclipsing binary systems
by: Prsa, Andrej
Published: (2025)

Constraining solar emission radius at 42 MHz during the 2024 total solar eclipse using a student-commissioned radio telescope
by: Young, Olivia R., et al.
Published: (2024)

Fundamental effective temperature measurements for eclipsing binary stars - VII. The solar twin in LL Aquarii
by: Miller, N. J., et al.
Published: (2025)

Modelling ion acceleration and transport in corotating interaction regions: the mass-to-charge ratio dependence of the particle spectrum
by: Ding, Zheyi, et al.
Published: (2024)

Starspots on eclipsing giant stars I.: The sample and eclipse mapping examples
by: Oláh, K., et al.
Published: (2025)

High-resolution spectroscopy of detached eclipsing binaries during total eclipses
by: Hełminiak, Krzysztof G., et al.
Published: (2024)

Rediscussion of eclipsing binaries. Paper XIX. The long-period solar-type system V454 Aurigae
by: Southworth, John
Published: (2024)