Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Lavorenti, Federico"'
Autor:
Lavorenti, Federico, Jensen, Elizabeth A., Aizawa, Sae, Califano, Francesco, D'Amore, Mario, Domingue, Deborah, Henri, Pierre, Lindsay, Simon, Raines, Jim M., Savin, Daniel Wolf
Mercury is the closest planet to the Sun, possesses a weak intrinsic magnetic field and has only a very tenuous atmosphere (exosphere). These three conditions result in a direct coupling between the plasma emitted from the Sun (namely the solar wind)
Externí odkaz:
http://arxiv.org/abs/2305.09498
Autor:
Lavorenti, Federico, Henri, Pierre, Califano, Francesco, Deca, Jan, Lindsay, Simon, Aizawa, Sae, Benkhoff, Johannes
Publikováno v:
A&A 674, A153 (2023)
Mercury is the archetype of a weakly magnetized, airless, telluric body immersed in the solar wind. Due to the lack of any substantial atmosphere, the solar wind directly precipitates on Mercury's surface. Using a 3D fully-kinetic self-consistent pla
Externí odkaz:
http://arxiv.org/abs/2209.08517
Autor:
Lavorenti, Federico, Henri, Pierre, Califano, Francesco, Deca, Jan, Aizawa, Sae, André, Nicolas, Benkhoff, Johannes
Publikováno v:
A&A 664, A133 (2022)
The planet Mercury possesses a small but highly dynamic magnetosphere in which the role and dynamics of electrons are still largely unknown. We aim at modeling the global dynamics of solar wind electrons impinging on Mercury's magnetosphere. Particul
Externí odkaz:
http://arxiv.org/abs/2205.00229
Autor:
Dargent, Jérémy, Lavorenti, Federico, Califano, Francesco, Henri, Pierre, Pucci, Francesco, Cerri, Silvio S.
Boundary layers in space and astrophysical plasmas are the location of complex dynamics where different mechanisms coexist and compete eventually leading to plasma mixing. In this work, we present fully kinetic Particle-In-Cell simulations of differe
Externí odkaz:
http://arxiv.org/abs/1911.00326
Akademický článek
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Akademický článek
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Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 652, pp.A20. ⟨10.1051/0004-6361/202141049⟩
Astronomy and Astrophysics-A&A, 2021, 652, pp.A20. ⟨10.1051/0004-6361/202141049⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 652, pp.A20. ⟨10.1051/0004-6361/202141049⟩
Astronomy and Astrophysics-A&A, 2021, 652, pp.A20. ⟨10.1051/0004-6361/202141049⟩
International audience; Context. Density inhomogeneities are ubiquitous in space and astrophysical plasmas, particularly at contact boundaries between different media. They often correspond to regions that exhibit strong dynamics across a wide range
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::bf49deb3d6255b65396c62a686b9c717
https://hal.archives-ouvertes.fr/hal-03313391
https://hal.archives-ouvertes.fr/hal-03313391