MB
Michaela Brchnelova
Netherlands Defence Academy, KU Leuven
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Solar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Stellar, planetary, and galactic studies
0000-0003-0874-2669
Employment
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NLDA Assistant Professor2025 - Present
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Katholieke Universiteit Leuven Doctoral Student2020 - 2024
Education
Education history is unavailable.
Projects & Funding
Projects & funding information is unavailable.
Publications (23)
- Performance of radio-based detection for operational monitoring of M5+ class solar flares Save
- Density-gradient-driven drift-wave turbulence in the solar corona Save
- Efficient magnetohydrodynamic modelling of the time-evolving corona by COCONUT Save
- A novel full MHD forecasting model chain from Sun to Earth: COCONUT+ Icarus Save
- Constraining the inner boundaries of COCONUT through plasma β and Alfvén speed Save
- Cross-field Diffusion Effects on Particle Transport in a Solar Coronal Flux Rope Save
- The operationally ready full 3D magnetohydrodynamic model from the Sun to Earth: COCONUT+Icarus Save
- Density-gradient-driven drift waves in the solar corona Save
- Modelling of Cryopumps for Space Electric Propulsion Usage Save
- Self-consistent propagation of flux ropes in realistic coronal simulations Save
- Magnetic connectivity from the Sun to the Earth: Impact of the magnetic modelling and input magnetic map Save
- Modelling the propagation of flux ropes in the coronal model COCONUT Save
- COCONUT, a Novel Fast-converging MHD Model for Solar Corona Simulations. II. Assessing the Impact of the Input Magnetic Map on Space-weather Forecasting at Minimum of Activity Save
- COCONUT, a Novel Fast-converging MHD Model for Solar Corona Simulations. III. Impact of the Preprocessing of the Magnetic Map on the Modeling of the Solar Cycle Activity and Comparison with Observations Save
- To E or Not to E : Numerical Nuances of Global Coronal Models Save
- COCONUT, a Novel Fast-converging MHD Model for Solar Corona Simulations: I. Benchmarking and Optimization of Polytropic Solutions Save
- Of mesh artefacts and electric fields: the bane of numerical global coronal modelling Save
- Effects of mesh topology on MHD solution features in coronal simulations Save
- Evaluations of Numerical Flux Schemes of a Coronal MHD Model Save
- Multi-ensemble MHD coronal modeling to improve background wind for CME propagation for EUHFORIA 2.0 Save