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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:scopusCancellation analysis of current density in solar active region NOAA10019
ArticleAbstract: Solar flares are often associated with changes in the fine magnetic structure of the emitting activePalabras claves:Active regions, Photosphere, Solar flaresAutores:Briand C., Carbone V., De Vita G., Lepreti F., Luca Sorriso-Valvo, Primavera L., Servidio S., Vecchio A.Fuentes:scopusKinetic electrostatic waves and their association with current structures in the solar wind
ArticleAbstract: Context. A variety of kinetic electrostatic and electromagnetic waves develop in the solar wind andPalabras 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., Píša D., Plettemeier D., Souček J., Steller M., Štverák , Trávníček P., Vaivads A., Vecchio A.Fuentes:scopusPeriodic behavior and stochastic fluctuations of solar activity: Proper orthogonal decomposition analysis
ArticleAbstract: We use the Proper Orthogonal Decomposition (POD) to investigate the spatiotemporal features of the sPalabras claves:Autores:Carbone V., Luca Sorriso-Valvo, Primavera L., Vecchio A.Fuentes:scopusPhase-synchronization, energy cascade, and intermittency in solar-wind turbulence
ArticleAbstract: The energy cascade in solar wind magnetic turbulence is investigated using MESSENGER data in the innPalabras claves:Autores:Bruno R., Carbone V., Korth H., Luca Sorriso-Valvo, Perri S., Vecchio A., Zurbuchen T.H.Fuentes:scopusProper orthogonal decomposition of solar photospheric motions
ArticleAbstract: The spatiotemporal dynamics of the solar photosphere is studied by performing a proper orthogonal dePalabras claves:Autores:Alfonsi G., Carbone V., Lepreti F., Luca Sorriso-Valvo, Primavera L., Straus T., Vecchio A., Veltri P.Fuentes:scopusPOD analysis of photospheric velocity field: Solar oscillations and granulation
Conference ObjectAbstract: The spatio-temporal dynamics of the solar photosphere is studied by performing a Proper Orthogonal DPalabras claves:Autores:Carbone V., Lepreti F., Luca Sorriso-Valvo, Straus T., Vecchio A., Veltri P.Fuentes:scopusSign singularity and flares in solar active region NOAA 11158
ArticleAbstract: Solar Active Region NOAA 11158 has hosted a number of strong flares, including one X2.2 event. The cPalabras claves:Sun: flares, Sun: magnetic fields, turbulence Supporting material: animationAutores:Carbone V., De Vita G., Fisher G.H., Kazachenko M.D., Krucker S., Lepreti F., Luca Sorriso-Valvo, Primavera L., Servidio S., Vecchio A., Welsch B.T.Fuentes:scopusStatistical study of electron density turbulence and ion-cyclotron waves in the inner heliosphere: Solar Orbiter observations
ArticleAbstract: Context. The recently released spacecraft potential measured by the RPW instrument on board Solar OrPalabras claves:plasmas, solar wind, Turbulence, WavesAutores:Angelini V., Bale S.D., Bruno R., Carbone F., Christian L. Vásconez, Chust T., D’Amicis R., 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 , Telloni D., Trávníček P., Vaivads A., Vecchio A., Yordanova E.Fuentes:googlescopusStudy of two interacting interplanetary coronal mass ejections encountered by Solar Orbiter during its first perihelion passage: Observations and modeling
ArticleAbstract: Context. Solar Orbiter, the new-generation mission dedicated to solar and heliospheric exploration,Palabras claves:magnetohydrodynamics (MHD), solar wind, Solar-terrestrial relations, Sun: coronal mass ejections (CMEs), Sun: evolution, Sun: heliosphereAutores:Adhikari L., Angelini V., Antonucci E., Bruno R., Carbone F., Chust T., Davies E.E., De Marco R., D’Amicis R., Evans V., Fineschi S., Giordano S., Gómez-Herrero R., Hietala H., Horbury T.S., Ivanovski S.L., Jagarlamudi V.K., Khotyaintsev Y.V., Kretzschmar M., Laker R., Liang H., Luca Sorriso-Valvo, Maksimovic M., Mancuso S., Messerotti M., Möstl C., Müller D., Nakanotani M., O'brien H., Perri S., Perrone D., Raffaele Marino, Reiss M.A., Rodríguez-Pacheco J., Romoli M., Scolini C., Souček J., Stangalini M., Steinvall K., Susino R., Telloni D., Vecchio A., Weiss A.J., Wimmer-Schweingruber R.F., Winslow R.M., Woodham L.D., Zank G.P., Zhao L.L., Zouganelis I.Fuentes:scopus