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Dissipation 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:googlescopusDifferential kinetic dynamics and heating of ions in the turbulent solar wind
ArticleAbstract: The solar wind plasma is a fully ionized and turbulent gas ejected by the outer layers of the solarPalabras claves:plasma heating, solar wind, space missions, TurbulenceAutores:Brienza D., Bruno R., Consolini G., de Keyser J., De Marco R., Lavraud B., Luca Sorriso-Valvo, Marcucci M.F., Perrone D., Pezzi O., Retinò A., Salatti M., Servidio S., Stabile S., Vaivads A., Valentini F., Veltri P.Fuentes:scopusFirst Solar Orbiter observation of the Alfvénic slow wind and identification of its solar source
ArticleAbstract: Context. Turbulence dominated by large-amplitude, nonlinear Alfvén-like fluctuations mainly propagatPalabras claves:Interplanetary medium, magnetohydrodynamics (MHD), methods: data analysis, solar wind, Sun: general, TurbulenceAutores:André N., Angelini V., Bruno R., Coco I., De Marco R., D’Amicis R., Evans V., Fedorov A., Genot V., Horbury T.S., Jagarlamudi V.K., Lavraud B., Livi S., Louarn P., Luca Sorriso-Valvo, Marcucci M.F., Matteini L., Müller D., O'brien H., Owen C.J., Panasenco O., Perrone D., Pezzi O., Rouillard A.P., Telloni D., Tenerani A., Velli M.C., Verscharen D., Woodham L.D., Zouganelis I.Fuentes:scopusImpact of Switchbacks on Turbulent Cascade and Energy Transfer Rate in the Inner Heliosphere
ArticleAbstract: Recent Parker Solar Probe (PSP) observations of inner heliospheric plasma have shown an abundant prePalabras claves:Autores:Bandyopadhyay R., Carlos S. Hernández, Chasapis A., Christian L. Vásconez, Luca Sorriso-Valvo, Pezzi O., Raffaele MarinoFuentes:scopusREVISITING A CLASSIC: The PARKER-MOFFATT PROBLEM
ArticleAbstract: The interaction of two colliding Alfvén wave packets is described here by means of magnetohydrodynamPalabras claves:magnetohydrodynamics (MHD), plasmas, solar windAutores:Christian L. Vásconez, Malara F., Matthaeus W.H., Parashar T.N., Pezzi O., Servidio S., Valentini F., Veltri P., Yang Y.Fuentes:googlescopusLocal 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:scopusProton-Proton Collisions in the Turbulent Solar Wind: Hybrid Boltzmann-Maxwell Simulations
ArticleAbstract: The mechanism of heating for hot, dilute, and turbulent plasmas represents a long-standing problem iPalabras claves:Autores:Luca Sorriso-Valvo, Perrone D., Pezzi O., Servidio S., Valentini F., Veltri P.Fuentes:scopusSign singularity of the local energy transfer in space plasma turbulence
ArticleAbstract: In weakly collisional space plasmas, the turbulent cascade provides most of the energy that is dissiPalabras claves:Dissipation, magnetosphere, Singularity, Space plasmas, TurbulenceAutores:Burch J.L., Catapano F., Chargazia K., Chen C.H.K., Christian L. Vásconez, De Vita G., Federico Fraternale, Giles B.L., Gurchumelia A., Kharshiladze O., Kvaratskhelia D., Le Conte O., Luca Sorriso-Valvo, Moore T.E., Nigro G., Perri S., Pezzi O., Retinò A., Torbert R.B., Yordanova E.Fuentes:googlescopusTransition to kinetic turbulence at proton scales driven by large-amplitude kinetic Alfvén fluctuations
ArticleAbstract: Space plasmas are dominated by the presence of large-amplitude waves, large-scale inhomogeneities, kPalabras claves:Interplanetary medium, plasmas, Turbulence, WavesAutores:Christian L. Vásconez, Malara F., Pezzi O., Pucci F., Servidio S., Valentini F.Fuentes:googlescopus