Recurrent release of coronal density structures during the rising phase of solar cycle 25

Aims. We investigate the main physical characteristics and outward propagation in the solar corona of small-scale coronal transients detected during the rising phase of solar activity cycle 25. They were observed with the Metis coronagraph on Solar Orbiter when the spacecraft was at perihelion, 0.29...

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Váldodahkkit:	Ventura R., Antonucci E., Spadaro D., Wang Y.-M., Romano P., Susino R., Guglielmino S. L., Nicolini G., Uslenghi M., Farina S., Abbo L., Burtovoi A., Casini C., De Leo Y., Frassati F., Jerse G., Landini F., Pancrazzi M., Romoli M., Russano G., Sasso C., Telloni D.
Materiálatiipa:	Artigo
Giella:	Inglês
Almmustuhtton:	EDP Sciences 2026-07-01
Ráidu:	Astronomy & Astrophysics
Fáttát:	magnetohydrodynamics (mhd) sun: corona solar wind
Liŋkkat:	https://www.aanda.org/articles/aa/full_html/2026/07/aa58403-25/aa58403-25.html
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