Five times the solar disk in a long row from left to right with main colors orange, light green, blue, green-red sprinkles, blue-to-red gradient, respresenting exemplary PMI data products after on-board analysis from left to right: continuum intensity, magnetic field strength, magnetic field inclination, magnetic field azimuth and line-of-sight velocity.

Publications of R. Bruno

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Journal Article (1)

1.
Journal Article
Telloni, D.; Antonucci, E.; Adhikari, L.; Zank, G. P.; Giordano, S.; Vai, M.; Zhao, L.-L.; Andretta, V.; Burtovoi, A.; Capuano, G. E. et al.; Da Deppo, V.; De Leo, Y.; Fineschi, S.; Grimani, C.; Heinzel, P.; Jerse, G.; Landini, F.; Liberatore, A.; Moses, J. D.; Naletto, G.; Nicolini, G.; Pancrazzi, M.; Romoli, M.; Russano, G.; Sasso, C.; Slemer, A.; Spadaro, D.; Stangalini, M.; Susino, R.; Teriaca, L.; Uslenghi, M.; Sorriso-Valvo, L.; Marino, R.; Perrone, D.; D'Amicis, R.; Bruno, R.: 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 and Astrophysics 670, p. L18 (2023)
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