Articolo in rivista, 2019, ENG, 10.1103/PhysRevLett.122.035102
Sorriso-Valvo, Luca; Catapano, Filomena; Retino, Alessandro; Le Contel, Olivier; Perrone, Denise; Roberts, Owen W.; Coburn, Jesse T.; Panebianco, Vincenzo; Valentini, Francesco; Perri, Silvia; Greco, Antonella; Malara, Francesco; Carbone, Vincenzo; Veltri, Pierluigi; Pezzi, Oreste; Fraternale, Federico; Di Mare, Francesca; Marino, Raffaele; Giles, Barbara; Moore, Thomas E.; Russell, Christopher T.; Torbert, Roy B.; Burch, Jim L.; Khotyaintsev, Yuri V.
UOS Cosenza; Escuela Politec Nacl; Univ Calabria; Sorbonne Univ; Imperial Coll London; Austrian Acad Sci; Gran Sasso Sci Inst; Politecn Torino; Univ Oslo; Univ Claude Bernard Lyon 1; NASA; Univ Calif Los Angeles; Univ Calif Los Angeles; Univ New Hampshire; Southwest Res Inst; Swedish Inst Space Phys
The description of the local turbulent energy transfer and the high-resolution ion distributions measured by the Magnetospheric Multiscale mission together provide a formidable tool to explore the cross-scale connection between the fluid-scale energy cascade and plasma processes at subion scales. When the small-scale energy transfer is dominated by Alfvenic, correlated velocity, and magnetic field fluctuations, beams of accelerated particles are more likely observed. Here, for the first time, we report observations suggesting the nonlinear wave-particle interaction as one possible mechanism for the energy dissipation in space plasmas.
Physical review letters (Print) 122 (3), pp. 035102-1–035102-8
Pezzi Oreste, Sorriso Valvo Luca
ID: 415456
Year: 2019
Type: Articolo in rivista
Creation: 2020-01-16 21:28:02.000
Last update: 2021-04-22 14:19:04.000
CNR authors
CNR institutes
External links
OAI-PMH: Dublin Core
OAI-PMH: Mods
OAI-PMH: RDF
DOI: 10.1103/PhysRevLett.122.035102
URL: https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.122.035102
External IDs
CNR OAI-PMH: oai:it.cnr:prodotti:415456
DOI: 10.1103/PhysRevLett.122.035102
ISI Web of Science (WOS): 000456782500006
Scopus: 2-s2.0-85060813683