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Magnetic turbulence in the geospace environment
ArticleAbstract: Magnetic turbulence is found in most space plasmas, including the Earth's magnetosphere, and the intPalabras claves:magnetosphere, Turbulence, Wave-particle interactionAutores:Aburjania G., Alexandrova O., Chargazia K., Greco A., Luca Sorriso-Valvo, Perri S., Vörös Z., Zimbardo G.Fuentes:scopusMethods for characterising microphysical processes in plasmas
ReviewAbstract: Advanced spectral and statistical data analysis techniques have greatly contributed to shaping our uPalabras claves:Data analysis methods, Plasma fluctuations, plasma turbulenceAutores:Alexandrova O., Dudok De Wit T., Furno I., Luca Sorriso-Valvo, Zimbardo G.Fuentes:scopusTurbulence Heating ObserveR - Satellite mission proposal
ArticleAbstract: The Universe is permeated by hot, turbulent, magnetized plasmas. Turbulent plasma is a major constitPalabras claves:plasma heating, plasma properties, Space plasma physicsAutores:Alexandrova O., André M., Bale S.D., Balikhin M., Burgess D., Camporeale E., Caprioli D., Chen C.H.K., Clacey E., Cully C.M., de Keyser J., Eastwood J.P., Eriksson S., Escoubet C.P., Fazakerley A.N., Goldstein M.L., Graham D.B., Haaland S., Hoshino M., Ji H., Karimabadi H., Khotyaintsev Y.V., Kucharek H., Lavraud B., Luca Sorriso-Valvo, Marcucci M.F., Matthaeus W.H., Moore T.E., Nakamura R., Narita Y., Nemecek Z., Norgren C., Opgenoorth H., Palmroth M., Perrone D., Pinçon J.L., Rathsman P., Retinò A., Rothkaehl H., Sahraoui F., Servidio S., Souček J., Vainio R., Vaivads A., Valentini F., Vörös Z., Wimmer-Schweingruber R.F.Fuentes:scopusScale-Dependent Kurtosis of Magnetic Field Fluctuations in the Solar Wind: A Multi-Scale Study With Cluster 2003–2015
ArticleAbstract: During the lifetime of the Cluster mission, the inter-spacecraft distances in the solar wind have chPalabras claves:Autores:Alexandrova O., Canu P., Escoubet C.P., Fischer D., Lion S., Luca Sorriso-Valvo, Nakamura R., Roberts O.W., Varsani A., Volwerk M., Vörös Z., Yearby K.Fuentes:scopusSmall-scale energy cascade of the solar wind turbulence
ArticleAbstract: Magnetic fluctuations in the solar wind are distributed according to Kolmogorov's power law f_5/3 bePalabras claves:MHD, solar wind, TurbulenceAutores:Alexandrova O., Carbone V., Luca Sorriso-Valvo, Veltri P.Fuentes:scopusSolar wind Cluster observations: Turbulent spectrum and role of Hall effect
ArticleAbstract: Turbulent spectrum of magnetic fluctuations in the solar wind nearly follows Kolmogorov's law ∼ f- 5Palabras claves:Interplanetary physics, Magnetohydrodynamics and plasmas, Space plasma physics, TurbulenceAutores:Alexandrova O., Carbone V., Luca Sorriso-Valvo, Veltri P.Fuentes:scopusSolar wind turbulence and the role of ion instabilities
ReviewAbstract: Solar wind is probably the best laboratory to study turbulence in astrophysical plasmas. In additionPalabras claves:Ion instabilities, Kinetic scales, plasma turbulence, solar windAutores:Alexandrova O., Bale S.D., Chen C.H.K., Horbury T.S., Luca Sorriso-ValvoFuentes:scopusSolar wind turbulent spectra and role of hall effect: A case study
Conference ObjectAbstract: Turbulent fluctuations within solar wind spectrum follows nearly Kolmogorov's power law spectrum f-5Palabras claves:ESA, LaTeX, MacrosAutores:Alexandrova O., Carbone V., Luca Sorriso-Valvo, Veltri P.Fuentes:scopusThe Solar Orbiter Science Activity Plan: Translating solar and heliospheric physics questions into action
ArticleAbstract: Solar Orbiter is the first space mission observing the solar plasma both in situ and remotely, fromPalabras claves:Methods: observational, Space vehicles: instruments, Sun: generalAutores:Abbo L., Alexandrova O., Anastasiadis A., Andretta V., Antonucci E., Appourchaux T., Aran A., Arge C.N., Auchère F., Aulanier G., Baker D., Bale S.D., Battaglia M., Bellot Rubio L., Bemporad A., Berghmans D., Berthomier M., Bocchialini K., Bonnin X., Brun A.S., Bruno R., Buchlin E., Büchner J., Bucik R., Carcaboso F., Carr R., Carrasco-Blázquez I., Cecconi B., Cernuda I., Chen C.H.K., Chitta L.P., Chust T., Dalmasse K., De Groof A., De Marco R., Deppo V.D., Dolei S., Dolla L., Dudok De Wit T., D’Amicis R., Eastwood J.P., Espinosa Lara F., Etesi L., Fedorov A., Félix-Redondo F., Fineschi S., Fleck B., Fludra A., Fontaine D., Fox N.J., Gandorfer A., Genot V., Georgoulis M.K., Gilbert H.R., Gissot S., Giunta A., Gizon L., Gómez-Herrero R., Gontikakis C., Graham G., Green L., Grundy T., Haberreiter M., Harra L.K., Hassler D.M., Hirzberger J., Ho G.C., Horbury T.S., Howard R.A., Hurford G., Innes D., Issautier K., James A.W., Janitzek N., Janvier M., Jeffrey N., Jenkins J., Khotyaintsev Y.V., Klein K.L., Kontar E.P., Kontogiannis I., Krafft C., Krasnoselskikh V., Krucker S., Lefort J., Luca Sorriso-Valvo, Maksimovic M., Müller D., Nieves-Chinchilla T., Osuna P., Owen C.J., Rodríguez-Pacheco J., Romoli M., Sanchez L., Solanki S.K., St Cyr O.C., Van Driel-Gesztelyi L., Walsh A.P., Watson C., Williams D.R., Zouganelis I.Fuentes:scopus