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Clustering of polarity reversals of the geomagnetic field
ArticleAbstract: Often in nature the temporal distribution of inhomogeneous stochastic point processes can be modeledPalabras claves:Autores:Carbone V., Guerra I., Harabaglia P., Lepreti F., Luca Sorriso-Valvo, Vecchio A., Veltri P.Fuentes:scopusA 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:scopusA statistical analysis of polarity reversals of the geomagnetic field
ArticleAbstract: We investigate the temporal distribution of polarity reversals of the geomagnetic field. In spite ofPalabras claves:Dynamo effect, Geomagnetism, Paleomagnetic measurementsAutores:Carbone V., Lepreti F., Luca Sorriso-Valvo, Nigro G., Stefani F., Vecchio A., Veltri P.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: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:scopusEnergetic ions in the Venusian system: Insights from the first Solar Orbiter flyby
ArticleAbstract: The Solar Orbiter flyby of Venus on 27 December 2020 allowed for an opportunity to measure the supraPalabras claves:acceleration of particles, Planet-star interactions, Planetary systems, Planets and satellites: terrestrial planets, Turbulence, WavesAutores:Allen R.C., Andrews G.B., Angelini V., Bale S.D., Berger L., Boden S., Böttcher S.I., Cernuda I., Chust T., Dimmock A.P., Eldrum S., Espada P.P., Espinosa Lara F., Evans V., Freiherr Von Forstner J.L., Gómez-Herrero R., Hadid L.Z., Hayes J.R., Hellín A.M., Ho G.C., Horbury T.S., Khotyaintsev Y.V., Kollhoff A., Krasnoselskikh V., Kretzschmar M., Kühl P., Kulkarni S.R., Lees W.J., Lorfèvre E., Luca Sorriso-Valvo, Maksimovic M., Martin C., Mason G.M., O'brien H., Pacheco D., Plettemeier D., Polo O.R., Prieto M., Ravanbakhsh A., Rodríguez-Pacheco J., Sánchez-Prieto S., Schlemm C.E., Seifert H., Souček J., Steller M., Stergiopoulou K., Štverák , Terasa J.C., Trávníček P., Tyagi K., Vaivads A., Vecchio A., Vines S.K., Volwerk M., Wimmer-Schweingruber R.F., Xu Z.G., Yedla M.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: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: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:scopus