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Alfvénicity-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:scopusErratum: On the occurrence of the third-order scaling in high-latitude solar wind (Astrophysical Journal (2012) 750 (41))
OtherAbstract:Palabras claves:Autores:Bruno R., Carbone V., D’Amicis R., Luca Sorriso-Valvo, Raffaele Marino, Veltri P.Fuentes:scopusDoes Turbulence along the Coronal Current Sheet Drive Ion Cyclotron Waves?
ArticleAbstract: Evidence for the presence of ion cyclotron waves (ICWs), driven by turbulence, at the boundaries ofPalabras claves:Autores:Adhikari L., Andretta V., Antonucci E., Bruno R., Burtovoi A., Carbone F., 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., Sasso C., Slemer A., Spadaro D., Stangalini M., Susino R., Telloni D., Teriaca L., Verscharen D., Zank G.P., Zhao L.L., Zimbardo G.Fuentes:scopusLinking Small-scale Solar Wind Properties with Large-scale Coronal Source Regions through Joint Parker Solar Probe-Metis/Solar Orbiter Observations
ArticleAbstract: The solar wind measured in situ by Parker Solar Probe in the very inner heliosphere is studied in coPalabras claves:Autores:Abbo L., Adhikari L., Andretta V., Auchère F., Bale S.D., Berlicki A., Biondo R., Bruno R., Capobianco G., Capuano G.E., Carbone F., Case A.W., Casini C., Casti M., Chioetto P., Ciaravella A., Corso A.J., Cuadrado R.A., Deppo V.D., Dudok De Wit T., D’Amicis R., Fabi M., Fineschi S., Frassati F., Frassetto F., Giordano S., Goetz K., Grimani C., Guglielmino S.L., Hadid L.Z., Harvey P.R., Heinzel P., Jerse G., Kasper J.C., Korreck K.E., Lamy P., Landini F., Lanzafame A., Larson D., Leo Y.D., Liang H., Liberatore A., Livi R., Luca Sorriso-Valvo, Macdowall R.J., Magli E., Malaspina D.M., Malvezzi M., Mancuso S., Massone G., Messerotti M., Moses J.D., Nakanotani M., Naletto G., Nicolini G., Nicolosi P., Nisticò G., Pagano P., Panasenco O., Pancrazzi M., Pelizzo M.G., Perrone D., Peter H., Pulupa M., Raffaele Marino, Reale F., Romano P., Romoli M., Sánchez-Cano B., Sasso C., Schühle U., Slemer A., Solanki S.K., Spadaro D., Stangalini M., Stevens M.L., Strachan L., Straus T., Susino R., Telloni D., Teriaca L., Tsinganos K., Uslenghi M., Velli M.C., Ventura R., Verscharen D., Vial J.C., Volpicelli C.A., Whittlesey P., Woch J., Zangrilli L., Zank G.P., Zhao L.L., Zimbardo G., Zuppella P.Fuentes:scopusRadial evolution of the intermittency of density fluctuations in the fast solar wind
ArticleAbstract: We study the radial evolution of the intermittency of density fluctuations in the fast solar wind. TPalabras claves:Interplanetary medium, magnetohydrodynamics (MHD), methods: data analysis, solar wind, WavesAutores:Bruno R., Carbone V., D’Amicis R., Luca Sorriso-Valvo, Malara F., Pietropaolo E., Primavera L., Telloni D., Veltri P.Fuentes:scopus