Výsledky vyhledávání - "Filippo Pantellini"

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Dynamics of energetic particles scattered in the solar wind: numerical simulations

Autor: Ahmed, Houeibib, Filippo, Pantellini, Lea, Griton

We propagate relativistic test particles in the field of a steady three-dimensional magnetohydrodynamic simulation of the solar wind. We use the MPI-AMRVAC code for the wind simulations and integrate the relativistic guiding center equations using a

Externí odkaz: http://arxiv.org/abs/2403.06706

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The Solar Orbiter Radio and Plasma Waves (RPW) instrument (Corrigendum)

Autor: Andris Vaivads, V. Krupař, M. Chariet, Lars Bylander, L. R. Malac-Allain, J. Parisot, Mats André, W. Recart, W. Puccio, C. Agrapart, D. Bérard, V. Leray, Robert F. Wimmer-Schweingruber, K. Boughedada, Baptiste Cecconi, E. Lorfèvre, M. Steller, B. Katra, F. Chapron, Helmut O. Rucker, Stuart D. Bale, Matthieu Kretzschmar, J.-C. Pellion, Ivana Kolmasova, J. Sanisidro, N. Quéruel, Filippo Pantellini, V. Bouzid, Laurent Lamy, Milan Maksimovic, L. Guéguen, C. Fiachetti, S. Chaintreuil, Mykhaylo Panchenko, Karine Issautier, M. Dekkali, O. Krupařová, Keith Goetz, Tomas Karlsson, I. Fratter, H. Ottacher, Philippe Louarn, P. Fergeau, O. Le Contel, Christopher J. Owen, Jan Soucek, A. Retino, Mihailo M. Martinović, Y. de Conchy, Olga Alexandrova, E. Bellouard, G. T. Delory, David Pisa, S. Thijs, E. Guilhem, Anders Eriksson, L. Åhlén, Antonio Vecchio, Timothy S. Horbury, Ondrej Santolik, Eduard P. Kontar, T. Vincent, V. Cripps, Daniel Dias, I. Zouganelis, A. Jeandet, T. Dudok de Wit, Sonny Lion, L. Uhlíř, Quynh Nhu Nguyen, M. Timofeeva, Dirk Plettemeier, J. Baše, Christopher Cully, Petr Hellinger, Lorenzo Matteini, Fouad Sahraoui, C. Collin, Paul Turin, Javier Rodriguez-Pacheco, Säm Krucker, P. Plasson, J.-Y. Brochot, Vladimir Krasnoselskikh, P. Leroy, Petr Travnicek, R. Lán, Yu. V. Khotyaintsev, S.-E. Jansson, Štěpán Štverák, G. Barbary, Pierre Astier, G. Jannet, R. Piberne, E. P. G. Johansson, F. Gonzalez, P. Danto, Arnaud Zaslavsky, J. Břínek, Thomas Chust, Xavier Bonnin, C. Laffaye, G. Cassam-Chenai, S. Julien, B. Pontet, Matthieu Berthomier

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 654, pp.C2. ⟨10.1051/0004-6361/201936214e⟩
Astronomy and Astrophysics-A&A, 2021, 654, pp.C2. ⟨10.1051/0004-6361/201936214e⟩
Astronomy & Astrophysics, 654, 1-2
Astronomy & Astrophysics, 654, pp. 1-2

Contains fulltext : 239392.pdf (Publisher’s version ) (Open Access)

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b30a16cb1d910cef89d7c1e436a533cd
https://hal.archives-ouvertes.fr/hal-03402816/file/aa36214e-19.pdf

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Fluid model of the plasma flow in the magnetic tail of a planet

Autor: Filippo Pantellini

All planets of the solar system with an active internal dynamo have a their magnetic dipole oriented perpendicularly or nearly perpendicularly to the solar wind during all or part of their orbit around the Sun. If, in addition, the planetary rotation

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::6c2338b70ef4010c0230477736528988
https://doi.org/10.5194/egusphere-egu21-7156

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3D MHD study of the Earth magnetosphere response during extreme space weather conditions

Autor: Victor Réville, S. Brun, Jacobo Varela Rodriguez, Antoine Strugarek, Filippo Pantellini, Philippe Zarka

The aim of the study is to analyze the response of the Earth magnetosphere for various space weather conditions and model the effect of interplanetary coronal mass ejections. The magnetopause stand off distance, open-closed field lines boundary and p

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::04d01fb78f866905d7a8ddca578e71ac
https://doi.org/10.5194/egusphere-egu21-1684

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Cross-comparison of global simulation models applied to Mercury's dayside magnetosphere

Autor: Jorge Amaya, Manabu Yagi, Vincent Génot, Léa Griton, Daniel Heyner, Filippo Pantellini, Shahab Fatemi, Hideyuki Usui, Jan Deca, Nicolas André, W. Exner, Sae Aizawa, Go Murakami

We present the first comparison of multiple global simulations of the solar wind interaction with Mercury’s dayside magnetosphere, conducted in the framework of the international collaborative project SHOTS - Studies on Hermean magnetosphere Orient

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::4ee1de89a29b3a4ee6d29258257c7dc3
https://doi.org/10.5194/epsc2020-261

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How a magnetic helix can develop at solstice in a Uranus-type rotating magnetosphere

Autor: Filippo Pantellini, Léa Griton

The characteristic relaxation time of the Uranus magnetosphere is of the order of the planet's rotation period. This is also the case for Jupiter or Saturn. However, the specificity of Uranus (and to a lesser extent of Neptune) is that the rotation a

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::a24841458d42cfecabdbfb9a6d937b24
https://doi.org/10.5194/epsc2020-731

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The Solar Orbiter Radio and Plasma Waves (RPW) instrument

Autor: L. R. Malac-Allain, T. Dudok de Wit, E. Lorfèvre, C. Collin, J. Sanisidro, Mihailo M. Martinović, X. Bonnin, E. Guilhem, Milan Maksimovic, P. Leroy, A. Vecchio, Eduard P. Kontar, L. Uhlíř, N. Quéruel, H. Ottacher, K. Boughedada, Christopher Cully, G. Barbary, Pierre Astier, Anders Eriksson, L. Åhlén, O. Krupařová, B. Pontet, T. Chust, G. Jannet, J. Parisot, Mats André, Paul Turin, P. Plasson, F. Chapron, M. Steller, W. Recart, W. Puccio, Vladimir Krasnoselskikh, Robert F. Wimmer-Schweingruber, V. Bouzid, Laurent Lamy, V. Cripps, R. Lán, Keith Goetz, B. Katra, S. Chaintreuil, Gregory T. Delory, I. Fratter, Dirk Plettemeier, C. Fiachetti, V. Krupař, M. Chariet, Sonny Lion, M. Dekkali, Lars Bylander, F. Gonzalez, Jan Soucek, Christopher J. Owen, Mykhaylo Panchenko, P. Danto, David Pisa, T. Vincent, Y. de Conchy, Säm Krucker, G. Cassam-Chenai, S. Julien, Baptiste Cecconi, Olga Alexandrova, A. Retino, V. Leray, Karine Issautier, S. Thijs, E. P. G. Johansson, Filippo Pantellini, D. Bérard, J. Baše, L. Guéguen, R. Piberne, P. Fergeau, Matthieu Berthomier, Tomas Karlsson, Arnaud Zaslavsky, Quynh Nhu Nguyen, J.-Y. Brochot, E. Bellouard, Yu. V. Khotyaintsev, Lorenzo Matteini, Štěpán Štverák, Javier Rodriguez-Pacheco, Fouad Sahraoui, S.-E. Jansson, O. Le Contel, Timothy S. Horbury, J.-C. Pellion, Pavel M. Trávníček, A. Jeandet, C. Agrapart, Petr Hellinger, Ondrej Santolik, I. Zouganelis, C. Laffaye, M. Timofeeva, D. Dias, Philippe Louarn, Helmut O. Rucker, Stuart D. Bale, Ivana Kolmasova, J. Břínek, Matthieu Kretzschmar, Andris Vaivads

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 642, pp.A12. ⟨10.1051/0004-6361/201936214⟩
Astronomy & Astrophysics, 642, pp. 1-23
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 642, pp.A12. ⟨10.1051/0004-6361/201936214⟩
Astronomy & Astrophysics, 642, 1-23

The Radio and Plasma Waves (RPW) instrument on the ESA Solar Orbiter mission is described in this paper. This instrument is designed to measure in-situ magnetic and electric fields and waves from the continuous to a few hundreds of kHz. RPW will also

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f4ea26a2173a44f0287dc43e97e89b38
https://hal.science/hal-02954313/file/aa36214-19.pdf

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MHD simulations of an Uranus type rotating magnetosphere

Autor: Filippo Pantellini, Léa Griton

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::48574de9e6155ee9ba50cc464230b3ba
https://doi.org/10.5194/egusphere-egu2020-18905

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A physical model for the magnetosphere of Uranus at solstice time

Autor: Filippo Pantellini

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 643, pp.A144. ⟨10.1051/0004-6361/202039143⟩

Uranus is the only planet in the Solar System whose rotation axis and orbital plane are nearly parallel to each other. Uranus is also the planet with the largest angle between the rotation axis and the direction of its magnetic dipole (roughly $59^\c

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::74fb898cfd7079d2b942fcdfb293f4ba

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MHD study of the planetary magnetospheric response during extreme solar wind conditions: Earth and exoplanet magnetospheres applications

Autor: Antoine Strugarek, Jacobo Varela, A. S. Brun, Philippe Zarka, Victor Réville, Filippo Pantellini

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 659, ⟨10.1051/0004-6361/202141181⟩

Context. The stellar wind and the interplanetary magnetic field modify the topology of planetary magnetospheres. Consequently, the hazardous effect of the direct exposition to the stellar wind, for example, regarding the integrity of satellites orbit

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::91f20f96972101fcd29ad36409b878fa
https://doi.org/10.1051/0004-6361/202141181

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