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

0571138 - ASÚ 2024 RIV FR eng J - Článek v odborném periodiku
Telloni, D. - Antonucci, E. - Adhikari, L. - Heinzel, Petr … celkem 36 autorů
First polar observations of the fast solar wind with the Metis Solar Orbiter coronagraph: Role of 2D turbulence energy dissipation in the wind acceleration.
Astronomy & Astrophysics. Roč. 670, February (2023), č. článku L18. ISSN 0004-6361. E-ISSN 1432-0746
Grant CEP: GA ČR(CZ) GA22-34841S
Institucionální podpora: RVO:67985815
Klíčová slova: magnetohydrodynamics * Sun * solar wind
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 6.5, rok: 2022
Způsob publikování: Open access

This Letter reports the first estimate of the expansion rate of polar coronal flows performed by the Metis coronagraph on board Solar Orbiter. By exploiting simultaneous measurements in polarized white light and ultraviolet intensity of the neutral hydrogen Lyman-α line, it was possible to extend observations of the outflow velocity of the main component of the solar wind from polar coronal holes out to 5.5 R⊙, the limit of diagnostic applicability and observational capabilities. We complement the results obtained with analogous polar observations performed with the UltraViolet Coronagraph Spectrometer on board the SOlar and Heliospheric Observatory during the previous full solar activity cycle, and find them to be satisfactorily reproduced by a magnetohydrodynamic turbulence model.
Trvalý link: https://hdl.handle.net/11104/0342430