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A possible truncated-Lévy-flight statistics recovered from interplanetary solar-wind velocity and magnetic-field fluctuations
ArticleAbstract: Interplanetary solar-wind fluctuations have been studied in the inner heliosphere and within the MHDPalabras claves:Autores:Bavassano B., Bruno R., Carbone V., Luca Sorriso-ValvoFuentes:scopusCoordinated study on solar wind turbulence during the venus-express, ACE and ulysses alignment of August 2007
Conference ObjectAbstract: At the end of August 2007, Venus, Earth and Ulysses were aligned within a few degrees. This unusualPalabras claves:MHD turbulence, solar wind, Space plasma physicsAutores:Baumjohann W., Bavassano B., Biernat H., Bruno R., Carbone V., Cattaneo M.B., D’Amicis R., Jankovičová D., Kovács P., Luca Sorriso-Valvo, Milillo A., Mura A., Orsini S., Rucker H., Veltri P., Vörös Z., Zhang T.Fuentes:scopusDensity fluctuations associated with turbulence and waves: First observations by Solar Orbiter
ArticleAbstract: Aims. The aim of this work is to demonstrate that the probe-to-spacecraft potential measured by RPWPalabras claves:solar wind, Turbulence, WavesAutores:Angelini V., Bale S.D., Chust T., Edberg N.J.T., Eriksson A.I., Evans V., Graham D.B., Horbury T.S., Johansson E.P.G., Khotyaintsev Y.V., Krasnoselskikh V., Kretzschmar M., Lorfèvre E., Luca Sorriso-Valvo, Maksimovic M., O'brien H., Plettemeier D., Souček J., Steinvall K., Steller M., Štverák , Trávníček P., Vaivads A., Vecchio A.Fuentes:scopusEditorial: Advances in Space Plasma Turbulence: Theory and Observations
OtherAbstract:Palabras claves:dissipation processes, in situ observations, magnetic reconnection, Numerical simulations, plasma turbulenceAutores:Hellinger P., Luca Sorriso-Valvo, Perri S., Tenerani A.Fuentes:scopusEditorial: New challenges in space plasma physics: Open questions and future mission concepts
OtherAbstract:Palabras claves:dissipation processes, in situ observations, magnetic reconnection, Numerical simulations, plasma turbulence, space physicsAutores:Chen C.H.K., Luca Sorriso-Valvo, Retinò A., Verscharen D.Fuentes:scopusHeating the solar wind by a magnetohydrodynamic turbulent energy cascade
ArticleAbstract: Solar wind plasma is known to cool down more slowly while it is blown away from the Sun than expectePalabras claves:MHD, solar wind, TurbulenceAutores:Bavassano B., Bruno R., Carbone V., Luca Sorriso-Valvo, Noullez A., Raffaele MarinoFuentes: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:scopusExploring the Solar Wind from Its Source on the Corona into the Inner Heliosphere during the First Solar Orbiter-Parker Solar Probe Quadrature
ArticleAbstract: This Letter addresses the first Solar Orbiter (SO)-Parker Solar Probe (PSP) quadrature, occurring onPalabras claves:Autores:Andretta V., Antonucci E., Auchère F., Bale S.D., Bemporad A., Bruno R., Capobianco G., Capuano G.E., Case A.W., Casini C., Casti M., Chioetto P., Corso A.J., De Leo Y., Deppo V.D., Dudok De Wit T., Fineschi S., Frassati F., Frassetto F., Giordano S., Goetz K., Guglielmino S.L., Habbal S., Harvey P.R., Heinzel P., Jerse G., Kasper J.C., Korreck K.E., Landini F., Larson D., Liberatore A., Livi R., Luca Sorriso-Valvo, Macdowall R.J., Magli E., Malaspina D.M., Massone G., Messerotti M., Moses J.D., Naletto G., Nicolini G., Nisticò G., Panasenco O., Pancrazzi M., Pelizzo M.G., Perrone D., Pinto R.F., Pulupa M., Reale F., Romano P., Romoli M., Sasso C., Schühle U., Spadaro D., Stangalini M., Stevens M.L., Strachan L., Straus T., Susino R., Telloni D., Teriaca L., Uslenghi M., Velli M.C., Verscharen D., Volpicelli C.A., Whittlesey P., Woodham L.D., Zangrilli L., Zank G.P., Zimbardo G., Zuppella 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: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:scopus