Mostrando 2 resultados de: 2
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:scopusTurbulence-Driven Ion Beams in the Magnetospheric Kelvin-Helmholtz Instability
ArticleAbstract: The description of the local turbulent energy transfer and the high-resolution ion distributions meaPalabras claves:Autores:Burch J.L., Carbone V., Catapano F., Coburn J.T., Di Mare F., Federico Fraternale, Giles B.L., Greco A., Khotyaintsev Y.V., Le Contel O., Luca Sorriso-Valvo, Malara F., Moore T.E., Panebianco V., Perri S., Perrone D., Pezzi O., Raffaele Marino, Retinò A., Roberts O.W., Russell C.T., Torbert R.B., Valentini F., Veltri P.Fuentes:scopus