AL
Andrea Lani
KU Leuven, Von Karman Institute for Fluid Dynamics, Universite Libre de Bruxelles École polytechnique de Bruxelles, Politecnico di Torino, Stanford University
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Computational Fluid Dynamics and Aerodynamics · Solar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics
0000-0003-4017-215X
Employment
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KU Leuven Research Expert2018 - Present
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Stanford University Postdoctoral fellow2010 - 2010
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Von Karman Institute For Fluid Dynamics Senior research engineer2008 - Present
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Von Karman Institute For Fluid Dynamics Researcher (Doctoral candidate)2002 - 2008
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Numeca International Development engineer2001 - 2002
Education
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Universite Libre de Bruxelles École polytechnique de Bruxelles Ph.D / Doctor in Engineering Sciences2003 - 2008
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Universite Libre de Bruxelles École polytechnique de Bruxelles Diplome d'Etudes Approfondies (DEA) in Applied Sciences2002 - 2003
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Politecnico di Torino M.Sc. in Aerospace Engineering1994 - 2000
Projects & Funding
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Virtual Space Weather Modeling Center (Part 2) European Space Agency2016 - 2018
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Ablation and Radiation in the presence of Light Ablators (ABLARADABLA) European Space Agency2015 - 2017
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Virtual Space Weather Modeling Center (Part 1) European Space Agency2012 - 2015
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CCN to "SIDC Data Exploitation" European Space Agency2012 - 2014
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Solar coronal mass ejections: innovative multi-component plasma Fonds Wetenschappelijk Onderzoek2011 - 2015
Publications (75)
- HelioFill: History-conditioned Diffusion Estimation of Solar Far-side EUV Emission Save
- The impact of the transition region in COCONUT Save
- Qorona: Open, Model-agnostic Line-of-sight Rendering of the Perpendicular Squashing Factor for Eclipse-like Coronal Imaging Save
- COCONUT: Towards practical time-evolving Sun-to-Earth magnetohydrodynamic modelling Save
- Revisiting magnetohydrodynamic modelling of the 2024 total solar eclipse with AI-reconstructed far-side photospheric field data Save
- MHD Modeling of Magnetic Flux Evolution Around Solar Maximum by the Coronal Model COCONUT Save
- On energy consistency of intermediate states in HLL-type MHD Riemann solvers Save
- Development of a High-order Flux Reconstruction Framework for Solar and Astrophysical Magnetohydrodynamics: Methods and Benchmarks Save
- COCONUT: A Coronal Model with an Energy Decomposition Strategy Save
- Modelling the total solar eclipse in 2024 with COCONUT Save
- SIP-IFVM: An Observation-based Magnetohydrodynamic Model of a Coronal Mass Ejection Save
- Experimental investigation on MHD flow manipulation in high enthalpy air plasma Save
- Time-evolving coronal modelling of the solar maximum around the solar storms in May 2024 by COCONUT Save
- SIP-IFVM: A Time-evolving Coronal Model with an Extended Magnetic Field Decomposition Strategy Save
- Toward High-order Solar Corona Simulations: A High-order Hyperbolized Poisson Approach for Magnetic Field Initialization Save
- Efficient magnetohydrodynamic modelling of the time-evolving corona by COCONUT Save
- Constraining the inner boundaries of COCONUT through plasma β and Alfvén speed Save
- Coronal mass ejection propagation in the dynamically coupled space weather tool: COCONUT + EUHFORIA Save
- SIP-IFVM: Efficient time-accurate magnetohydrodynamic model of the corona and coronal mass ejections Save
- Dependence of coronal mass ejections on the morphology and toroidal flux of their source magnetic flux ropes Save