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scopus(4)
Building up Solar-wind-like 3D Uniform-intensity Magnetic Fields
ArticleAbstract: A numerical model representing a 3D turbulent constant-magnitude magnetic field B is described. AssuPalabras claves:Magnetic fields, solar wind, TurbulenceAutores:Bruno R., Luca Sorriso-Valvo, Malara F., Primavera L., Valentini F.Fuentes:scopusOn the estimation of the current density in space plasmas: Multi- versus single-point techniques
ArticleAbstract: Thanks to multi-spacecraft mission, it has recently been possible to directly estimate the current dPalabras claves:Electric current vector, Multi-spacecraft technique, Space plasmasAutores:Luca Sorriso-Valvo, Malara F., Perri S., Reda A., Valentini F.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:scopusTwo-fluid numerical simulations of turbulence inside Kelvin-Helmholtz vortices: Intermittency and reconnecting current sheets
ArticleAbstract: The turbulence developing inside Kelvin-Helmholtz vortices has been studied using a two-fluid numeriPalabras claves:Autores:Califano F., Chasapis A., Henri P., Luca Sorriso-Valvo, Retinò A., Rezeau L., Rossi C., Servidio S., Valentini F.Fuentes:scopus