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pro vyhledávání: '"Khiar, Benjamin"'
Autor:
Levesque, Joseph M., Liao, Andy S., Hartigan, Patrick, Young, Rachel P., Trantham, Matthew, Klein, Sallee, Gray, William, Manuel, Mario, Fiksel, Gennady, Katz, Joseph, Li, Chikang, Birkel, Andrew, Tzeferacos, Petros, Hansen, Edward C., Khiar, Benjamin, Foster, John M., Kuranz, Carolyn
Publikováno v:
Published in Physics of Plasmas 29, 012106 (2022)
The magnetic field produced by planets with active dynamos, like the Earth, can exert sufficient pressure to oppose supersonic stellar wind plasmas, leading to the formation of a standing bow shock upstream of the magnetopause, or pressure-balance su
Externí odkaz:
http://arxiv.org/abs/2201.03520
Autor:
Yao, Weipeng, Capitaine, Julien, Khiar, Benjamin, Vinci, Tommaso, Burdonov, Konstantin, Béard, Jérôme, Fuchs, Julien, Ciardi, Andrea
Magnetized laser-produced plasmas are central to many new studies in laboratory astrophysics, inertial confinement fusion, and industrial applications. Here we present the results of large-scale, three-dimensional magneto-hydrodynamic simulations of
Externí odkaz:
http://arxiv.org/abs/2105.13800
Autor:
Khiar, Benjamin
Nous présentons dans ce travail différentes configurations utilisées pour étudier des éxperiences, pertinentes d'un point de vue astrophysique, mettant en jeu des plasma produits par laser ainsi que des champs magnétiques intenses. les outils t
Externí odkaz:
http://www.theses.fr/2017PA066310/document
Akademický článek
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Autor:
Revet, Guilhem, Chen, Sophia N., Bonito, Rosaria, Khiar, Benjamin, Filippov, Evgeny, Argiroffi, Costanza, Higginson, Drew P., Orlando, Salvatore, Béard, Jérôme, Blecher, Marius, Borghesi, Marco, Burdonov, Konstantin, Khaghani, Dimitri, Naughton, Kealan, Pépin, Henri, Portugall, Oliver, Riquier, Raphael, Rodriguez, Rafael, Ryazantsev, Sergei N., Yu. Skobelev, Igor, Soloviev, Alexander, Willi, Oswald, Pikuz, Sergey, Ciardi, Andrea, Fuchs, Julien
Publikováno v:
Science Advances
Science Advances, American Association for the Advancement of Science (AAAS), 2017, 3 (11), pp.e1700982. ⟨10.1126/sciadv.1700982⟩
Science Advances, 2017, 3 (11), pp.e1700982. ⟨10.1126/sciadv.1700982⟩
Science Advances, American Association for the Advancement of Science (AAAS), 2017, 3 (11), pp.e1700982. ⟨10.1126/sciadv.1700982⟩
Science Advances, 2017, 3 (11), pp.e1700982. ⟨10.1126/sciadv.1700982⟩
When matter accretes onto a young star, a shell of dense material can form around the impact, reducing its x-ray emission.
Accretion dynamics in the formation of young stars is still a matter of debate because of limitations in observations and
Accretion dynamics in the formation of young stars is still a matter of debate because of limitations in observations and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid_dedup__::5624936ad8109f593f8558956e6b5589
https://hal-cea.archives-ouvertes.fr/cea-01887635
https://hal-cea.archives-ouvertes.fr/cea-01887635
Autor:
Revet, G., Chen, S. N., Bonito, Rosaria, Khiar, Benjamin, Filippov, E., argiroffi, costanza, Higginson, D.P., orlando, salvatore, Beard, J., Blecher, marius, Borghesi, Marco, Naughton, Kealan, Chen, Shenchang, Burdonov, Konstantin, Khaghani, D., Pépin, H., Portugall, O., Riquier, R., Rodriguez, Rafael, Ryazantsev, Sergey, Skobelev, I. Yu., Soloviev, A., Willi, Oswald, Pikuz, S. A., Ciardi, A., Fuchs, J.
Publikováno v:
Revet, G, Chen, S N, Bonito, R, Khiar, B, Filippov, E, argiroffi, C, Higginson, D P, orlando, S, Beard, J, Blecher, M, Borghesi, M, Naughton, K, Chen, S, Burdonov, K, Khaghani, D, Pépin, H, Portugall, O, Riquier, R, Rodriguez, R, Ryazantsev, S, Skobelev, I Y, Soloviev, A, Willi, O, Pikuz, S A, Ciardi, A & Fuchs, J 2017, ' Laboratory unraveling of matter accretion in young stars ', Science Advances, vol. 3, no. 11, e1700982, pp. 1-10 . https://doi.org/10.1126/sciadv.1700982
Accretion dynamics in the formation of young stars is still a matter of debate because of limitations in observations and modeling. Through scaled laboratory experiments of collimated plasma accretion onto a solid in the presence of a magnetic field,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2607::c33941ee0617a4c6cb7f903dec4a88ba
https://pure.qub.ac.uk/en/publications/d6ce0514-bd51-44f9-aefa-c85aa403eed5
https://pure.qub.ac.uk/en/publications/d6ce0514-bd51-44f9-aefa-c85aa403eed5
Autor:
Khiar, Benjamin
Publikováno v:
Astrophysics [astro-ph]. Université Pierre et Marie Curie-Paris VI, 2017. English. ⟨NNT : 2017PA066310⟩
We present in this work different configurations used as a mean to study astrophysically-relevant (by scaling) experiments using laser-produced plasmas and strong magnetic fields. This work is a contribution to the relatively recent field known as hi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::93605f9e616a820442a393b024865361
https://tel.archives-ouvertes.fr/tel-01699030v2/document
https://tel.archives-ouvertes.fr/tel-01699030v2/document
Autor:
Revet G; Institute of Applied Physics, 46 Ulyanov Street, 603950 Nizhny Novgorod, Russia.; LULI (Laboratoire pour l'Utilisation des Lasers Intenses)-CNRS, École Polytechnique; Commissariat à l'Energie Atomique et aux Energies Alternatives (CEA), Université Paris-Saclay; Sorbonne Universités, Universite Pierre et Marie Curie (UPMC) Paris 06, F-91128 Palaiseau cedex, France., Chen SN; Institute of Applied Physics, 46 Ulyanov Street, 603950 Nizhny Novgorod, Russia.; LULI (Laboratoire pour l'Utilisation des Lasers Intenses)-CNRS, École Polytechnique; Commissariat à l'Energie Atomique et aux Energies Alternatives (CEA), Université Paris-Saclay; Sorbonne Universités, Universite Pierre et Marie Curie (UPMC) Paris 06, F-91128 Palaiseau cedex, France., Bonito R; INAF (Istituto Nazionale di Astrofisica)-Osservatorio Astronomico di Palermo, Palermo, Italy.; Dipartimento di Fisica e Chimica, Università di Palermo, Palermo, Italy., Khiar B; Sorbonne Universités, UPMC Paris 06, Observatoire de Paris, PSL (Paris Sciences et Lettre) Research University, CNRS, UMR 8112, LERMA (Laboratoire d'Etudes du Rayonnement et de la Matière en Astrophysique), F-75005 Paris, France., Filippov E; National Research Nuclear University MEPhI (Moscow Engineering Physics Institute), Moscow 115409, Russia.; Joint Institute for High Temperatures, RAS (Russian Academy of Sciences), Moscow 125412, Russia., Argiroffi C; Dipartimento di Fisica e Chimica, Università di Palermo, Palermo, Italy., Higginson DP; LULI (Laboratoire pour l'Utilisation des Lasers Intenses)-CNRS, École Polytechnique; Commissariat à l'Energie Atomique et aux Energies Alternatives (CEA), Université Paris-Saclay; Sorbonne Universités, Universite Pierre et Marie Curie (UPMC) Paris 06, F-91128 Palaiseau cedex, France.; Lawrence Livermore National Laboratory, Livermore, CA 94551, USA., Orlando S; INAF (Istituto Nazionale di Astrofisica)-Osservatorio Astronomico di Palermo, Palermo, Italy., Béard J; LNCMI (Laboratoire National des Champs Magnétiques Intenses), UPR 3228, CNRS-UGA-UPS-INSA, Toulouse 31400, France., Blecher M; Institut für Laser- und Plasmaphysik, Heinrich-Heine-Universität Düsseldorf, D-40225 Düsseldorf, Germany., Borghesi M; Centre for Plasma Physics, Queen's University of Belfast, Belfast BT7 1NN, UK., Burdonov K; Institute of Applied Physics, 46 Ulyanov Street, 603950 Nizhny Novgorod, Russia., Khaghani D; GSI (Gesellschaft für Schwerionenforschung) Helmholtzzentrum für Schwerionenforschung GmbH, 64291 Darmstadt, Germany., Naughton K; Centre for Plasma Physics, Queen's University of Belfast, Belfast BT7 1NN, UK., Pépin H; INRS-EMT (Institut National de la Recherche Scientifique, Énergie, Matériaux et Télécommunication), Varennes, Québec, Canada., Portugall O; LNCMI (Laboratoire National des Champs Magnétiques Intenses), UPR 3228, CNRS-UGA-UPS-INSA, Toulouse 31400, France., Riquier R; LULI (Laboratoire pour l'Utilisation des Lasers Intenses)-CNRS, École Polytechnique; Commissariat à l'Energie Atomique et aux Energies Alternatives (CEA), Université Paris-Saclay; Sorbonne Universités, Universite Pierre et Marie Curie (UPMC) Paris 06, F-91128 Palaiseau cedex, France.; CEA, DAM, DIF (Commissariat à l'Energie Atomique Energie Atomique, Direction des Applications Militaires Île de France), 91297 Arpajon, France., Rodriguez R; Departamento de Fisica de la Universidad de Las Palmas de Gran Canaria, E-35017 Las Palmas de Gran Canaria, Spain., Ryazantsev SN; Joint Institute for High Temperatures, RAS (Russian Academy of Sciences), Moscow 125412, Russia., Yu Skobelev I; National Research Nuclear University MEPhI (Moscow Engineering Physics Institute), Moscow 115409, Russia.; Joint Institute for High Temperatures, RAS (Russian Academy of Sciences), Moscow 125412, Russia., Soloviev A; Institute of Applied Physics, 46 Ulyanov Street, 603950 Nizhny Novgorod, Russia., Willi O; Institut für Laser- und Plasmaphysik, Heinrich-Heine-Universität Düsseldorf, D-40225 Düsseldorf, Germany., Pikuz S; National Research Nuclear University MEPhI (Moscow Engineering Physics Institute), Moscow 115409, Russia.; Joint Institute for High Temperatures, RAS (Russian Academy of Sciences), Moscow 125412, Russia., Ciardi A; Sorbonne Universités, UPMC Paris 06, Observatoire de Paris, PSL (Paris Sciences et Lettre) Research University, CNRS, UMR 8112, LERMA (Laboratoire d'Etudes du Rayonnement et de la Matière en Astrophysique), F-75005 Paris, France., Fuchs J; Institute of Applied Physics, 46 Ulyanov Street, 603950 Nizhny Novgorod, Russia.; LULI (Laboratoire pour l'Utilisation des Lasers Intenses)-CNRS, École Polytechnique; Commissariat à l'Energie Atomique et aux Energies Alternatives (CEA), Université Paris-Saclay; Sorbonne Universités, Universite Pierre et Marie Curie (UPMC) Paris 06, F-91128 Palaiseau cedex, France.
Publikováno v:
Science advances [Sci Adv] 2017 Nov 01; Vol. 3 (11), pp. e1700982. Date of Electronic Publication: 2017 Nov 01 (Print Publication: 2017).