First polar observations of the fast solar wind with the Metis Solar Orbiter coronagraph: Role of 2D turbulence energy dissipation in the wind acceleration

Article

Abstract: Context. The fast solar wind is known to emanate from polar coronal holes. Aims. This Letter reports

Palabras claves:

magnetohydrodynamics (MHD), solar wind, Sun: corona, Sun: UV radiation

Autores:

Adhikari L., Andretta V., Antonucci E., Bruno R., Burtovoi A., Capuano G.E., 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., Russano G., Sasso C., Slemer A., Spadaro D., Stangalini M., Susino R., Telloni D., Teriaca L., Uslenghi M., Vai M., Zank G.P., Zhao L.L.

Fuentes:

scopus