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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Detaylı Bibliyografya
Asıl Yazarlar:	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.
Materyal Türü:	Artigo
Dil:	Inglês
Baskı/Yayın Bilgisi:	EDP Sciences 2026-07-01
Seri Bilgileri:	Astronomy & Astrophysics
Konular:	magnetohydrodynamics (mhd) sun: corona solar wind
Online Erişim:	https://www.aanda.org/articles/aa/full_html/2026/07/aa58403-25/aa58403-25.html
Etiketler:	Etiketle Etiket eklenmemiş, İlk siz ekleyin!

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

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