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Astronomy and Astrophysics(1)
Astrophysical Journal(1)
Monthly Notices of the Royal Astronomical Society(1)
New Journal of Physics(1)
First 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: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: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: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:googlescopus