BP
Barbara Perri
CEA Paris-Saclay, KU Leuven, Université Versailles Saint-Quentin-en-Yvelines, École Nationale Supérieure de Techniques Avancées Paris, IAS, Université Paris-Sud
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Solar and Space Plasma Dynamics · Stellar, planetary, and galactic studies · Ionosphere and magnetosphere dynamics
0000-0002-2137-2896
Employment
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CEA Saclay Deputy Astronomer2022 - Present
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KU Leuven Post-Doc2020 - 2022
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IAS Junior Post-Doc2019 - 2020
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CEA Saclay PhD Student2016 - 2019
- 2015 - 2015
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Thales Group (Germany) Intern2014 - 2014
Education
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Université Versailles Saint-Quentin-en-Yvelines Master2015 - 2016
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ENSTA ParisTech Engineering Degree2013 - 2016
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Université Paris-Sud Bachelor2013 - 2014
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Lycée Richelieu High School Diploma2008 - 2011
Projects & Funding
Projects & funding information is unavailable.
Publications (29)
- Active nests at solar maximum: How nested flux emergence dominated flaring activity and structured the heliosphere Save
- Far-side active region emergence catalogue from Solar Orbiter/PHI Save
- A prolific solar flare factory Save
- Activity of low-mass stars in the light of spot signature in the Fourier domain Save
- An Open Platform for Validating Ambient Solar Wind Models Save
- Magnetic connectivity from the Sun to the Earth with MHD models Save
- Impact of far-side structures observed by Solar Orbiter on coronal and heliospheric wind simulations Save
- Impact of the Solar Activity on the Propagation of ICMEs: Simulations of Hydro, Magnetic and Median ICMEs at the Minimum and Maximum of Activity Save
- Self-consistent propagation of flux ropes in realistic coronal simulations Save
- Bottlenecks in space weather model validation: Where do we stand and how do we move forward? Save
- Magnetic connectivity from the Sun to the Earth: Impact of the magnetic modelling and input magnetic map 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
- Validation of a Wave Heated 3D MHD Coronal-wind Model using Polarized Brightness and EUV Observations 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
- Powering Stellar Magnetism: Energy Transfers in Cyclic Dynamos of Sun-like Stars Save