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Colliding Alfvénic wave packets in magnetohydrodynamics, Hall and kinetic simulations
ArticleAbstract: The analysis of the Parker-Moffatt problem, recently revisited in Pezzi et al. (Astrophys. J., vol.Palabras claves:Astrophysical Plasmas, Plasma Simulation, Space plasma physicsAutores:Christian L. Vásconez, Malara F., Matthaeus W.H., Parashar T.N., Pezzi O., Servidio S., Valentini F., Veltri P., Yang Y.Fuentes:googlescopusNonlinear waves and instabilities leading to secondary reconnection in reconnection outflows
ArticleAbstract: Reconnection outflows have been under intense recent scrutiny, from in situ observations and from siPalabras claves:Astrophysical Plasmas, Plasma Simulation, Space plasma physicsAutores:Goldman M.V., Lapenta G., Luca Sorriso-Valvo, Newman D.L., Olshevsky V., Pucci F., Servidio S.Fuentes:scopusLocal and global properties of energy transfer in models of plasma turbulence
ArticleAbstract: The nature of the turbulent energy transfer rate is studied using direct numerical simulations of wePalabras claves:plasma nonlinear phenomena, Plasma Simulation, Space plasma physicsAutores:Christian L. Vásconez, Laveder D., Luca Sorriso-Valvo, Mininni P.D., Perrone D., Raffaele Marino, Servidio S., Valentini F.Fuentes:scopusLocal energy transfer rate and kinetic processes: The fate of turbulent energy in two-dimensional hybrid Vlasov-Maxwell numerical simulations
ArticleAbstract: The nature of the cross-scale connections between the inertial-range turbulent energy cascade and thPalabras claves:plasma nonlinear phenomena, Plasma Simulation, Space plasma physicsAutores:Luca Sorriso-Valvo, Perrone D., Pezzi O., Servidio S., Valentini F., Veltri P., Zouganelis I.Fuentes:scopusTurbulence Heating ObserveR - Satellite mission proposal
ArticleAbstract: The Universe is permeated by hot, turbulent, magnetized plasmas. Turbulent plasma is a major constitPalabras claves:plasma heating, plasma properties, Space plasma physicsAutores:Alexandrova O., André M., Bale S.D., Balikhin M., Burgess D., Camporeale E., Caprioli D., Chen C.H.K., Clacey E., Cully C.M., de Keyser J., Eastwood J.P., Eriksson S., Escoubet C.P., Fazakerley A.N., Goldstein M.L., Graham D.B., Haaland S., Hoshino M., Ji H., Karimabadi H., Khotyaintsev Y.V., Kucharek H., Lavraud B., Luca Sorriso-Valvo, Marcucci M.F., Matthaeus W.H., Moore T.E., Nakamura R., Narita Y., Nemecek Z., Norgren C., Opgenoorth H., Palmroth M., Perrone D., Pinçon J.L., Rathsman P., Retinò A., Rothkaehl H., Sahraoui F., Servidio S., Souček J., Vainio R., Vaivads A., Valentini F., Vörös Z., Wimmer-Schweingruber R.F.Fuentes:scopus