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A simple model for the solar cycle
ArticleAbstract: A simple nonlinear model which describes the 11 -year solar cycle can be derived from the usual α -Palabras claves:Autores:Carbone V., Lepreti F., Luca Sorriso-Valvo, Pontieri A., Vecchio A.Fuentes:scopusArbitrary-order Hilbert Spectral Analysis and Intermittency in Solar Wind Density Fluctuations
ArticleAbstract: The properties of inertial- and kinetic-range solar wind turbulence have been investigated with thePalabras claves:plasmas, solar wind, TurbulenceAutores:Alberti T., Carbone F., Chen C.H.K., Lepreti F., Luca Sorriso-Valvo, Nemecek Z., Šafránková J.Fuentes:scopusFirst polar observations of the fast solar wind with the Metis Solar Orbiter coronagraph: Role of 2D turbulence energy dissipation in the wind acceleration
ArticleAbstract: Context. The fast solar wind is known to emanate from polar coronal holes. Aims. This Letter reportsPalabras claves:magnetohydrodynamics (MHD), solar wind, Sun: corona, Sun: UV radiationAutores:Adhikari L., Andretta V., Antonucci E., Bruno R., Burtovoi A., Capuano G.E., De Leo Y., Deppo V.D., D’Amicis R., Fineschi S., Giordano S., Grimani C., Heinzel P., Jerse G., Landini F., Liberatore A., Luca Sorriso-Valvo, Moses J.D., Naletto G., Nicolini G., Pancrazzi M., Perrone D., Raffaele Marino, Romoli M., Russano G., Sasso C., Slemer A., Spadaro D., Stangalini M., Susino R., Telloni D., Teriaca L., Uslenghi M., Vai M., Zank G.P., Zhao L.L.Fuentes:scopusDifferential 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:scopusMultifractal analysis of high resolution solar wind proton density measurements
ArticleAbstract: The solar wind is a highly turbulent medium, with a high level of field fluctuations throughout a brPalabras claves:Multifractal, solar wind, TurbulenceAutores:Carbone F., Chen C.H.K., Leonardis E., Luca Sorriso-Valvo, Nemecek Z., Šafránková J.Fuentes:scopusMultipoint observation of anisotropy and intermittency in solar-wind turbulence
ArticleAbstract: Using high-resolution magnetic-field Cluster observations, we have investigated the magnetic-field aPalabras claves:Autores:Carbone V., Luca Sorriso-Valvo, Perri S., Yordanova E.Fuentes:scopusHelios 2 observations of solar wind turbulence decay in the inner heliosphere
ArticleAbstract: Aims. A linear scaling of the mixed third-order moment of the magnetohydrodynamic (MHD) fluctuationsPalabras claves:magnetohydrodynamics (MHD), solar wind, TurbulenceAutores:Bruno R., D,Aamicis R., Foldes R., Lévêque E., Luca Sorriso-Valvo, Raffaele Marino, Telloni D., Yordanova E.Fuentes:scopusICARUS: in-situ studies of the solar corona beyond Parker Solar Probe and Solar Orbiter
ArticleAbstract: The primary scientific goal of ICARUS (Investigation of Coronal AcceleRation and heating of solar wiPalabras claves:Heliophysics, Solar atmosphere, solar wind, Space missionAutores:Agapitov O., Balat-Pichelin M., Bale S.D., Balikhin M., Baumjohann W., Berthomier M., Bruno R., Cranmer S.R., de Pontieu B., Dudok De Wit T., Eastwood J., Erdelyi R., Ergun R., Fedorov A., Fedun V., Ganushkina N., Greco A., Harra L.K., Henri P., Horbury T.S., Hudson H., Kasper J., Khotyaintsev Y.V., Krasnoselskikh V., Kretzschmar M., Krucker S., Kucharek H., Langevin Y., Lavraud B., Lebreton J.P., Lepri S., Liemohn M., Louarn P., Luca Sorriso-Valvo, Maksimovic M., Meneses D.d.S., Moebius E., Mozer F., Nemecek Z., Panasenco O., Retinò A., Šafránková J., Scudder J., Servidio S., Souček J., Szabo A., Tsurutani B.T., Vaivads A., Vekstein G., Velli M.C., Vörös Z., Walker S., Zaqarashvili T., Zimbardo G.Fuentes:scopusObservation of a Magnetic Switchback in the Solar Corona
ArticleAbstract: Switchbacks are sudden, large radial deflections of the solar wind magnetic field, widely revealed iPalabras claves:Autores:Adhikari L., Andretta V., Antonucci E., Auchère F., Berghmans D., Biondo R., Bruno R., Burtovoi A., Capuano G.E., Carbone F., Casini C., Casti M., Chioetto P., Chitta L.P., Cuadrado R.A., De Leo Y., Deppo V.D., Downs C., D’Amicis R., Fabi M., Fineschi S., Frassati F., Giarrusso M., Grimani C., Harra L.K., Heinzel P., Jerse G., Kraaikamp E., Landini F., Liang H., Liberatore A., Long D.M., Luca Sorriso-Valvo, Mancuso S., Mandal S., Moses J.D., Nakanotani M., Naletto G., Nicolini G., Pancrazzi M., Parenti S., Pelouze G., Perrone D., Peter H., Raffaele Marino, Rodriguez L., Romoli M., Russano G., Sasso C., Schühle U., Schwanitz C., Smith P.J., Spadaro D., Stangalini M., Susino R., Telloni D., Teriaca L., Verbeeck C., Zank G.P., Zhao L.L., Zhukov A.N.Fuentes:scopusObservations of turbulence and anomalous scaling in the solar wind
ArticleAbstract: In situ observations collected in the past decades, at different heliocentric distances and coveringPalabras claves:MHD turbulence, scaling, solar windAutores:Bavassano B., Bruno R., Carbone V., D’Amicis R., Luca Sorriso-Valvo, Noullez A., Raffaele Marino, Salem C.Fuentes:scopus