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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:scopusAlfvénicity-related Long Recovery Phases of Geomagnetic Storms: A Space Weather Perspective
ReviewAbstract: This paper reports, for the first time on a statistical basis, on the key role played by the AlfvéniPalabras claves:Autores:Bruno R., Choraghe K., D’Amicis R., Luca Sorriso-Valvo, Perrone D., Raghav A.N., Telloni D.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:scopusEvolution of Solar Wind Turbulence from 0.1 to 1 au during the First Parker Solar Probe-Solar Orbiter Radial Alignment
ArticleAbstract: The first radial alignment between Parker Solar Probe and Solar Orbiter spacecraft is used to investPalabras claves:Autores:Adhikari L., Angelini V., Antonucci E., Bale S.D., Bruno R., Carbone F., Case A.W., De Marco R., Dudok De Wit T., D’Amicis R., Evans V., Goetz K., Harvey P.R., Horbury T.S., Jagarlamudi V.K., Kasper J.C., Korreck K.E., Laker R., Larson D., Liang H., Livi R., Livi S., Louarn P., Luca Sorriso-Valvo, Macdowall R.J., Malaspina D.M., Nakanotani M., O'brien H., Owen C.J., Panasenco O., Perrone D., Pulupa M., Raffaele Marino, Romoli M., Shi C., Steinvall K., Stevens M.L., Telloni D., Tenerani A., Velli M.C., Whittlesey P., Woodham L.D., 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:scopusMultiscale views of an Alfvénic slow solar wind: 3D velocity distribution functions observed by the Proton-Alpha Sensor of Solar Orbiter
ArticleAbstract: Context. The Alfvénic slow solar wind is of particular interest, as it is often characterized by intPalabras claves:plasmas, solar wind, TurbulenceAutores:Allegrini F., André N., Angelini V., Bale S.D., Barthe A., Berthomier M., Bruno R., D’Amicis R., Evans V., Fedorov A., Fortunato V., Fruit G., Genot V., Horbury T.S., Kasper J.C., Khataria D., Kieokaew R., Lavraud B., Livi S., Louarn P., Luca Sorriso-Valvo, Maksimovic M., Mele G., O'brien H., Owen C.J., Penou E., Plotnikov I., Prech L., Raines J.M., Réville V., Rouillard A.P., Verscharen D.Fuentes:scopusNo Evidence for Critical Balance in Field-aligned Alfvénic Solar Wind Turbulence
ArticleAbstract: The properties of Alfvénic solar wind turbulence have been studied for decades using spacecraft measPalabras claves:Autores:Adhikari L., Bruno R., Carbone F., Hunana P., Luca Sorriso-Valvo, Telloni D., Zank G.P.Fuentes:scopusObservation and Modeling of the Solar Wind Turbulence Evolution in the Sub-Mercury Inner Heliosphere
ArticleAbstract: This letter exploits the radial alignment between the Parker Solar Probe and BepiColombo in late 202Palabras claves:Autores:Adhikari L., Alberti T., Auster H.U., Bale S.D., Bruno R., Califano F., Carbone F., Case A.W., Dudok De Wit T., D’Amicis R., Goetz K., Grimani C., Hadid L.Z., Harvey P.R., Heyner D., Kasper J.C., Korreck K.E., Laker R., Larson D., Liberatore A., Livi R., Luca Sorriso-Valvo, Macdowall R.J., Malara F., Malaspina D.M., Milillo A., Narita Y., Panasenco O., Perrone D., Pulupa M., Raffaele Marino, Richter I., Sánchez-Cano B., Shi C., Stawarz J.E., Stevens M.L., Susino R., Telloni D., Velli M.C., Verdini A., Verscharen D., Whittlesey P., Zank G.P., Zhao L.L.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:scopus