Zobrazeno 1 - 10
of 252
pro vyhledávání: '"Filippov E"'
Autor:
Scisciò, M., Petringa, G., Zhu, Z., Rodrigues, M. R. D., Alonzo, M., Andreoli, P. L., Filippi, F., Consoli, Fe., Huault, M., Raffestin, D., Molloy, D., Larreur, H., Singappuli, D., Carriere, T., Verona, C., Nicolai, P., McNamee, A., Ehret, M., Filippov, E., Lera, R., Pérez-Hernández, J. A., Agarwal, S., Krupka, M., Singh, S., Istokskaia, V., Lattuada, D., La Cognata, M., Guardo, G. L., Palmerini, S., Rapisarda, G., Batani, K., Cipriani, M., Cristofari, G., Di Ferdinando, E., Di Giorgio, G., De Angelis, R., Giulietti, D., Xu, J., Volpe, L., Rodríguez-Frías, M. D., Giuffrida, L., Margarone, D., Batani, D., Cirrone, G. A. P., Bonasera, A., Consoli, Fa.
Driving the nuclear fusion reaction p+11B -> 3 alpha + 8.7 MeV in laboratory conditions, by interaction between high-power laser pulses and matter, has become a popular field of research, due to numerous applications that it can potentially allow: an
Externí odkaz:
http://arxiv.org/abs/2411.04577
Autor:
Sladkov, A., Fegan, C., Yao, W., Bott, A. F. A., Chen, S. N., Ahmed, H., Filippov, E. D., Lelièvre, R., Martin, P., McIlvenny, A., Waltenspiel, T., Antici, P., Borghesi, M., Pikuz, S., Ciardi, A., d'Humières, E., Soloviev, A., Starodubtsev, M., Fuchs, J.
Interactions between magnetic fields advected by matter play a fundamental role in the Universe at a diverse range of scales. A crucial role these interactions play is in making turbulent fields highly anisotropic, leading to observed ordered fields.
Externí odkaz:
http://arxiv.org/abs/2404.12110
Autor:
Fazzini, A., Yao, W., Burdonov, K., Béard, J., Chen, S. N., Ciardi, A., d'Humières, E., Diab, R., Filippov, E. D., Kisyov, S., Lelasseux, V., Miceli, M., Moreno, Q., Orlando, S., Pikuz, S., Ribeyre, X., Starodubtsev, M., Zemskov, R., Fuchs, J.
Colliding collisionless shocks appear in a great variety of astrophysical phenomena and are thought to be possible sources of particle acceleration in the Universe. To investigate the detailed dynamics of this phenomenon, we have performed a dedicate
Externí odkaz:
http://arxiv.org/abs/2202.03465
Autor:
Burdonov, K., Fazzini, A., Lelasseux, V., Albrecht, J., Antici, P., Ayoul, Y., Beluze, A., Cavanna, D., Ceccotti, T., Chabanis, M., Chaleil, A., Chen, S. N., Chen, Z., Consoli, F., Cuciuc, M., Davoine, X., Delaneau, J. P., d'Humières, E., Dubois, J-L., Evrard, C., Filippov, E., Freneaux, A., Forestier-Colleoni, P., Gremillet, L., Horny, V., Lancia, L., Lecherbourg, L., Lebas, N., Leblanc, A., Ma, W., Martin, L., Negoita, F., Paillard, J-L., Papadopoulos, D., Perez, F., Pikuz, S., Qi, G., Quéré, F., Ranc, L., Söderstrom, P. -A., Scisciò, M., Sun, S., Vallières, S., Wang, P., Yao, W., Mathieu, F., Audebert, P., Fuchs, J.
We present the results of the first commissioning phase of the ``short focal length'' area (SFA) of the Apollon laser facility (located in Saclay, France), which was performed with the first available laser beam (F2), scaled to a nominal power of one
Externí odkaz:
http://arxiv.org/abs/2108.01336
Autor:
Yao, W., Fazzini, A., Chen, S. N., Burdonov, K., Antici, P., Béard, J., Bolaños, S., Ciardi, A., Diab, R., Filippov, E. D., Kisyov, S., Lelasseux, V., Miceli, M., Moreno, Q., Nastasa, V., Orlando, S., Pikuz, S., Popescu, D. C., Revet, G., Ribeyre, X., d'Humières, E., Fuchs, J.
Collisionless shocks are ubiquitous in the Universe and are held responsible for the production of non-thermal particles and high-energy radiation. In the absence of particle collisions in the system, theoretical works show that the interaction of an
Externí odkaz:
http://arxiv.org/abs/2104.12170
Autor:
Yao, W., Fazzini, A., Chen, S. N., Burdonov, K., Antici, P., Béard, J., Bolaños, S., Ciardi, A., Diab, R., Filippov, E. D., Kisyov, S., Lelasseux, V., Miceli, M., Moreno, Q., Nastasa, V., Orlando, S., Pikuz, S., Popescu, D. C., Revet, G., Ribeyre, X., d'Humières, E., Fuchs, J.
Charged particles can be accelerated to high energies by collisionless shock waves in astrophysical environments, such as supernova remnants. By interacting with the magnetized ambient medium, these shocks can transfer energy to particles. Despite in
Externí odkaz:
http://arxiv.org/abs/2011.00135
Autor:
Filippov, E. D., Makarov, S. S., Burdonov, K. F., Yao, W., Revet, G., Béard, J., Bolaños, S., Chen, S. N., Guediche, A., Hare, J., Romanovsky, D., Skobelev, I. Yu., Starodubtsev, M., Ciardi, A., Pikuz, S. A., Fuchs, J.
We analyze, using experiments and 3D MHD numerical simulations, the dynamics and radiative properties of a plasma ablated by a laser (1 ns, 10$^{12}$-10$^{13}$ W/cm$^2$) from a solid target, as it expands into a homogeneous, strong magnetic field (up
Externí odkaz:
http://arxiv.org/abs/2006.12424
Autor:
Revet, G., Khiar, B., Filippov, E., Argiroffi, C., Béard, J., Bonito, R., Cerchez, M., Chen, S. N., Gangolf, T., Higginson, D. P., Mignone, A., Olmi, B., Ouillé, M., Ryazantsev, S. N., Skobelev, I. Yu., Safronova, M. I., Starodubtsev, M., Vinci, T., Willi, O., Pikuz, S., Orlando, S., Ciardi, A., Fuchs, J.
The shaping of astrophysical outflows into bright, dense and collimated jets due to magnetic pressure is here investigated using laboratory experiments. We notably look at the impact on jet collimation of a misalignment between the outflow, as it ste
Externí odkaz:
http://arxiv.org/abs/2004.09840
Autor:
Khiar, B., Revet, G., Ciardi, A., Burdonov, K., Filippov, E., Béard, J., Cerchez, M., Chen, S. N., Gangolf, T., Makarov, S. S., Ouillé, M., Safronova, M., Skobelev, I. Yu., Soloviev, A., Starodubtsev, M., Willi, O., Pikuz, S., Fuchs, J.
Publikováno v:
Phys. Rev. Lett. 123, 205001 (2019)
Magnetized laser-produced plasmas are central to many novel laboratory astrophysics and inertial confinement fusion studies, as well as in industrial applications. Here we provide the first complete description of the three-dimensional dynamics of a
Externí odkaz:
http://arxiv.org/abs/1910.13778
Autor:
Bolanos, S., Smets, R., Chen, S. N., Grisolet, A., Filippov, E., Henares, J. L, Nastasa, V., Pikuz, S., Riquier, R., Safranova, M., Severin, A., Starodubtsev, M., Fuchs, J.
Magnetic reconnection occurs when two plasmas having co-planar but anti-parallel magnetic fields meet. At the contact point, the field is locally annihilated and the magnetic energy can be released into the surrounding plasma. Theory and numerical mo
Externí odkaz:
http://arxiv.org/abs/1909.01684