Vlasov-Poisson simulations of strong wave-plasma interaction of relevance for radiofrequency plasma heating (Articolo in rivista)

Type
Label
  • Vlasov-Poisson simulations of strong wave-plasma interaction of relevance for radiofrequency plasma heating (Articolo in rivista) (literal)
Anno
  • 1999-01-01T00:00:00+01:00 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#doi
  • 10.1103/PhysRevLett.83.96 (literal)
Alternative label
  • Francesco Califano (1) and Maurizio Lontano (2) (1999)
    Vlasov-Poisson simulations of strong wave-plasma interaction of relevance for radiofrequency plasma heating
    in Physical review letters
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • Francesco Califano (1) and Maurizio Lontano (2) (literal)
Pagina inizio
  • 96 (literal)
Pagina fine
  • 99 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#url
  • http://prl.aps.org/abstract/PRL/v83/i1/p96_1 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
  • 83 (literal)
Rivista
Note
  • ISI Web of Science (WOS) (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
  • (1) Istituto Nazionale Fisica della Materia, Sezione A, Università di Pisa, Italy (2) Istituto di Fisica del Plasma \"Piero Caldirola,\" C.N.R., EURATOM-ENEA-CNR Association, Milan, Italy (literal)
Titolo
  • Vlasov-Poisson simulations of strong wave-plasma interaction of relevance for radiofrequency plasma heating (literal)
Abstract
  • The nonlinear aspects of the interaction between externally applied electrostatic oscillations and a one-dimensional electron-ion plasma is investigated by numerically integrating the Vlasov-Poisson system of equations. The forcing held is in the form of a broad symmetric k spectrum which simulates that used in low-frequency wave-heating experiments in tokamak plasmas. It is shown that, for realistic values of the plasma and field parameters, numerous nonlinear effects accompany the wave-plasma interaction, as, for example, the formation of density cavities by the action of ponderomotive forces, the acceleration of charged particles, and the nonlinear plasma heating. (literal)
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