Mostrando 3 resultados de: 3
First Solar Orbiter observation of the Alfvénic slow wind and identification of its solar source
ArticleAbstract: Context. Turbulence dominated by large-amplitude, nonlinear Alfvén-like fluctuations mainly propagatPalabras claves:Interplanetary medium, magnetohydrodynamics (MHD), methods: data analysis, solar wind, Sun: general, TurbulenceAutores:André N., Angelini V., Bruno R., Coco I., De Marco R., D’Amicis R., Evans V., Fedorov A., Genot V., Horbury T.S., Jagarlamudi V.K., Lavraud B., Livi S., Louarn P., Luca Sorriso-Valvo, Marcucci M.F., Matteini L., Müller D., O'brien H., Owen C.J., Panasenco O., Perrone D., Pezzi O., Rouillard A.P., Telloni D., Tenerani A., Velli M.C., Verscharen D., Woodham L.D., Zouganelis I.Fuentes:scopusMultiscale views of an Alfvénic slow solar wind: 3D velocity distribution functions observed by the Proton-Alpha Sensor of Solar Orbiter
ArticleAbstract: Context. The Alfvénic slow solar wind is of particular interest, as it is often characterized by intPalabras claves:plasmas, solar wind, TurbulenceAutores:Allegrini F., André N., Angelini V., Bale S.D., Barthe A., Berthomier M., Bruno R., D’Amicis R., Evans V., Fedorov A., Fortunato V., Fruit G., Genot V., Horbury T.S., Kasper J.C., Khataria D., Kieokaew R., Lavraud B., Livi S., Louarn P., Luca Sorriso-Valvo, Maksimovic M., Mele G., O'brien H., Owen C.J., Penou E., Plotnikov I., Prech L., Raines J.M., Réville V., Rouillard A.P., Verscharen D.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