Zobrazeno 1 - 10
of 643
pro vyhledávání: '"A Retinò"'
Autor:
Barbhuiya, M. Hasan, Cassak, Paul A., Chasapis, Alex, Shay, Michael A., Cozzani, Giulia, Retino, Alessandro
Magnetic reconnection often initiates abruptly and then rapidly progresses to a nonlinear quasi-steady state. While satellites frequently detect reconnection events, ascertaining whether the system has achieved steady-state or is still evolving in ti
Externí odkaz:
http://arxiv.org/abs/2410.14139
Autor:
Pecora, Francesco, Pucci, Francesco, Malara, Francesco, Klein, Kristopher G., Marcucci, Maria Federica, Retinò, Alessandro, Matthaeus, William
Plasma turbulence involves complex, nonlinear interactions of electromagnetic fields and charged particles across multiple scales. Studying these phenomena in space plasmas, like the solar wind, is facilitated by the intrinsic scale separations and t
Externí odkaz:
http://arxiv.org/abs/2407.06679
Autor:
Retino, A., Kepko, L., Kucharek, H., Marcucci, M. F., Nakamura, R., Amano, T., Angelopoulos, V., Bale, S. D., Caprioli, D., Cassak, P., Chasapis, A., Chen, L. -J., Dai, L., Dunlop, M. W., Forsyth, C., Fu, H., Galvin, A., Contel, O. Le, Yamauchi, M., Kistler, L., Khotyaintsev, Y., Klein, K., Mann, I. R., Matthaeus, W., Mouikis, K., Nykyri, K., Palmroth, M., Plaschke, F., Saito, Y., Soucek, J., Spence, H., Turner, D. L., Vaivads, A., Valentini, F.
Energetic plasma is everywhere in the Universe. The terrestrial Magnetospheric System is a key case where direct measures of plasma energization and energy transport can be made in situ at high resolution. Despite the large amount of available observ
Externí odkaz:
http://arxiv.org/abs/2311.09920
Autor:
Klein, Kristopher G., Spence, Harlan, Alexandrova, Olga, Argall, Matthew, Arzamasskiy, Lev, Bookbinder, Jay, Broeren, Theodore, Caprioli, Damiano, Case, Anthony, Chandran, Benjamin, Chen, Li-Jen, Dors, Ivan, Eastwood, Jonathan, Forsyth, Colin, Galvin, Antoinette, Genot, Vincent, Halekas, Jasper, Hesse, Michael, Hine, Butler, Horbury, Tim, Jian, Lan, Kasper, Justin, Kretzschmar, Matthieu, Kunz, Matthew, Lavraud, Benoit, Contel, Olivier Le, Mallet, Alfred, Maruca, Bennett, Matthaeus, William, Niehof, Jonathan, O'Brian, Helen, Owen, Christopher, Retino, Alessandro, Reynolds, Christopher, Roberts, Owen, Schekochihin, Alexander, Skoug, Ruth, Smith, Charles, Smith, Sonya, Steinberg, John, Stevens, Michael, Szabo, Adam, TenBarge, Jason, Torbert, Roy, Vasquez, Bernard, Verscharen, Daniel, Whittlesey, Phyllis, Wickizer, Brittany, Zank, Gary, Zweibel, Ellen
HelioSwarm (HS) is a NASA Medium-Class Explorer mission of the Heliophysics Division designed to explore the dynamic three-dimensional mechanisms controlling the physics of plasma turbulence, a ubiquitous process occurring in the heliosphere and in p
Externí odkaz:
http://arxiv.org/abs/2306.06537
Autor:
Goodrich, Katherine, Schwartz, Steven, Wilson III, Lynn, Cohen, Ian, Turner, Drew, Caspi, Amir, Smith, Keith, Rose, Randall, Whittlesey, Phyllis, Plaschke, Ferdinand, Halekas, Jasper, Hospodarsky, George, Burch, James, Gingell, Imogen, Chen, Li-Jen, Retino, Alessandro, Khotyaintsev, Yuri
Publikováno v:
Bulletin of the AAS, Vol. 55, Issue 3, Whitepaper #134 (9pp); 2023 July 31
Collisionless shock waves are one of the main forms of energy conversion in space plasmas. They can directly or indirectly drive other universal plasma processes such as magnetic reconnection, turbulence, particle acceleration and wave phenomena. Col
Externí odkaz:
http://arxiv.org/abs/2306.05491
Autor:
Trotta, Domenico, Pezzi, Oreste, Burgess, David, Preisser, Luis, Blanco-Cano, Xochitl, Kajdic, Primoz, Hietala, Heli, Horbury, Timothy S., Vainio, Rami, Dresing, Nina, Retino', Alessandro, Marcucci, Maria Federica, Sorriso-Valvo, Luca, Servidio, Sergio, Valentini, Francesco
The complex interaction between shocks and plasma turbulence is extremely important to address crucial features of energy conversion in a broad range of astrophysical systems. We study the interaction between a supercritical, perpendicular shock and
Externí odkaz:
http://arxiv.org/abs/2305.15168
Autor:
Matthaeus, W. H., Adhikari, S., Bandyopadhyay, R., Brown, M. R., Bruno, R., Borovsky, J., Carbone, V., Caprioli, D., Chasapis, A., Chhiber, R., Dasso, S., Dmitruk, P., Del Zanna, L., Dmitruk, P. A., Franci, Luca, Gary, S. P., Goldstein, M. L., Gomez, D., Greco, A., Horbury, T. S., Ji, Hantao, Kasper, J. C., Klein, K. G., Landi, S., Li, Hui, Malara, F., Maruca, B. A., Mininni, P., Oughton, Sean, Papini, E., Parashar, T. N., Pecora, F., Petrosyan, Arakel, Pouquet, Annick, Retino, A., Roberts, Owen, Ruffolo, David, Servidio, Sergio, Spence, Harlan, Smith, C. W., Stawarz, J. E., TenBarge, Jason, Vasquez, B. J., Vaivads, Andris, Valentini, F., Velli, Marco, Verdini, A., Verscharen, Daniel, Whittlesey, Phyllis, Wicks, Robert, Yang, Y., Zimbardo, G.
Space plasmas are three-dimensional dynamic entities. Except under very special circumstances, their structure in space and their behavior in time are not related in any simple way. Therefore, single spacecraft in situ measurements cannot unambiguous
Externí odkaz:
http://arxiv.org/abs/2211.12676
Autor:
F Valentini, D Perrone, S Stabile, O Pezzi, S Servidio, R De Marco, F Marcucci, R Bruno, B Lavraud, J De Keyser, G Consolini, D Brienza, L Sorriso-Valvo, A Retinò, A Vaivads, M Salatti, P Veltri
Publikováno v:
New Journal of Physics, Vol 18, Iss 12, p 125001 (2016)
The solar wind plasma is a fully ionized and turbulent gas ejected by the outer layers of the solar corona at very high speed, mainly composed by protons and electrons, with a small percentage of helium nuclei and a significantly lower abundance of h
Externí odkaz:
https://doaj.org/article/9ac42af10ea24b5d8634d6953101a690
Autor:
Verscharen, D., Wicks, R. T., Branduardi-Raymont, G., Erdélyi, R., Frontera, F., Götz, C., Guidorzi, C., Lebouteiller, V., Matthews, S. A., Nicastro, F., Rae, I. J., Retinò, A., Simionescu, A., Soffitta, P., Uttley, P., Wimmer-Schweingruber, R. F.
Publikováno v:
Front. Astron. Space Sci. 8:651070 (2021)
In review of the White Papers from the Voyage 2050 process and after the public presentation of a number of these papers in October 2019 in Madrid, we as White Paper lead authors have identified a coherent science theme that transcends the divisions
Externí odkaz:
http://arxiv.org/abs/2104.07983
Autor:
Graham, D. B., Khotyaintsev, Yu. V., André, M., Vaivads, A., Chasapis, A., Matthaeus, W. H., Retino, A., Valentini, F., Gershman, D. J.
Plasmas in Earth's outer magnetosphere, magnetosheath, and solar wind are essentially collisionless. This means particle distributions are not typically in thermodynamic equilibrium and deviate significantly from Maxwellian distributions. The deviati
Externí odkaz:
http://arxiv.org/abs/2102.09639