First Solar Orbiter observation of the Alfvénic slow wind and identification of its solar source

Article

Abstract: Context. Turbulence dominated by large-amplitude, nonlinear Alfvén-like fluctuations mainly propagat

Palabras claves:

Interplanetary medium, magnetohydrodynamics (MHD), methods: data analysis, solar wind, Sun: general, Turbulence

Autores:

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:

scopus