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Slow wind belt in the quiet solar corona
DOI: 10.1063/5.0132824 Bibcode: 2023PhPl...30b2905A

Romoli, M.; Andretta, V.; Uslenghi, M. +16 more

The slow solar wind belt in the quiet corona, observed with the Metis coronagraph on board Solar Orbiter on May 15, 2020, during the activity minimum of the cycle 24, in a field of view extending from 3.8 R ⊙ to 7.0 R ⊙, is formed by a slow and dense wind stream running along the coronal current sheet, accelerating in the radial direction and reac…

2023 Physics of Plasmas
SolarOrbiter 10
Unexpected energetic particle observations near the Sun by Parker Solar Probe and Solar Orbiter
DOI: 10.1063/5.0147683 Bibcode: 2023PhPl...30e0501M

McComas, D. J.; Rodríguez-Pacheco, J.; Wimmer-Schweingruber, R. F. +6 more

Solar energetic particles (SEPs) from suprathermal (few keV) up to relativistic (∼few GeV) energies are accelerated at the Sun in association with solar flares and coronal mass ejection-driven shock waves. Although our knowledge of the origin, acceleration, and transport of these particles from close to the Sun through the interplanetary medium ha…

2023 Physics of Plasmas
SolarOrbiter 5