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Evolution 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: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:scopusStudy 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