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Astrophysical Journal(4)
Journal of Plasma Physics(2)
Monthly Notices of the Royal Astronomical Society(2)
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Journal of Geophysical Research: Space Physics(1)
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Electricidad y electrónica(5)
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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:googlescopusFrom Alfvén waves to kinetic Alfvén waves in an inhomogeneous equilibrium structure
ArticleAbstract: Kinetic Alfvén waves are believed to primary form fluctuations in a hydromagnetic turbulence at scalPalabras claves:Alfvén waves, Hall MHD, kinetic Alfvén waves, kinetic plasma simulations, solar coronaAutores:Christian L. Vásconez, Malara F., Matthaeus W.H., Pezzi O., Pucci F., Servidio S., Valentini F.Fuentes:googlescopusGeneration of Turbulence in Colliding Reconnection Jets
ArticleAbstract: The collision of magnetic reconnection jets is studied by means of a three-dimensional numerical simPalabras claves:magnetic reconnection, methods: numerical, TurbulenceAutores:Chasapis A., Goldman M.V., Lapenta G., Luca Sorriso-Valvo, Matthaeus W.H., Newman D.L., Olshevsky V., Pucci F., Servidio S.Fuentes:scopusDissipation measures in weakly collisional plasmas
ArticleAbstract: The physical foundations of the dissipation of energy and the associated heating in weakly collisionPalabras claves:magnetic reconnection, plasmas, solar wind, TurbulenceAutores:Cassak P.A., Christian L. Vásconez, Juno J.L., Liang H., Luca Sorriso-Valvo, Matthaeus W.H., Perrone D., Pezzi O., Roytershteyn V., Servidio S., TenBarge J.M.Fuentes:googlescopusParticle energization in space plasmas: towards a multi-point, multi-scale plasma observatory
ArticleAbstract: This White Paper outlines the importance of addressing the fundamental science theme “How are chargePalabras claves:Astrophysical Plasmas, Heliosphere, Particle energization, Scale coupling, Space plasmas, Spacecraft constellationsAutores:Angelopoulos V., Blasi P., Burch J.L., Dai L., de Keyser J., Dunlop M., Eastwood J.P., Fu H., Haaland S., Hoshino M., Johlander A., Kepko L., Khotyaintsev Y.V., Kucharek H., Lapenta G., Lavraud B., Le Contel O., Luca Sorriso-Valvo, Malandraki O.E., Marcucci M.F., Matthaeus W.H., McWilliams K., Petrukovich A., Pinçon J.L., Plaschke F., Retinò A., Saito Y., Vainio R., Vaivads A., Wimmer-Schweingruber R.F.Fuentes:scopusIn Situ Observation of Hall Magnetohydrodynamic Cascade in Space Plasma
ArticleAbstract: We present estimates of the turbulent energy-cascade rate derived from a Hall-magnetohydrodynamic (MPalabras claves:Autores:Bandyopadhyay R., Burch J.L., Chasapis A., Franci L., Gershman D.J., Giles B.L., Hellinger P., Landi S., Luca Sorriso-Valvo, Matteini L., Matthaeus W.H., Moore T.E., Pollock C.J., Russell C.T., Strangeway R.J., Torbert R.B., Verdini A.Fuentes:scopusKINETIC ALFVÉN WAVE GENERATION by LARGE-SCALE PHASE MIXING
ArticleAbstract: One view of the solar wind turbulence is that the observed highly anisotropic fluctuations at spatiaPalabras claves:lasmas, solar wind, Sun: corona, WavesAutores:Christian L. Vásconez, Malara F., Matthaeus W.H., Pucci F., Servidio S., Valentini F.Fuentes:googlescopusTurbulence 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:scopusScale dependence of energy transfer in turbulent plasma
ArticleAbstract: In the context of space and astrophysical plasma turbulence and particle heating, several vocabulariPalabras claves:MHD, plasmas, solar wind, TurbulenceAutores:Chen S., Lu Q., Luca Sorriso-Valvo, Matthaeus W.H., Parashar T.N., Shi Y., Wan M., Yang Y.Fuentes:scopusVelocity-space cascade in magnetized plasmas: Numerical simulations
ArticleAbstract: Plasma turbulence is studied via direct numerical simulations in a two-dimensional spatial geometry.Palabras claves:Autores:Greco A., Luca Sorriso-Valvo, Matthaeus W.H., Perrone D., Pezzi O., Servidio S., Valentini F., Veltri P.Fuentes:scopus