Supergranulation and Poleward Migration of the Magnetic Field at High Latitudes of the Sun

Magnetoconvection at the solar surface governs the dynamics in the upper solar atmosphere and sustains the heliosphere. Properties of this fundamental process are poorly described near the solar poles. Here we report the first out-of-ecliptic remote-sensing observations of the south pole of the Sun...

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Ngā kaituhi matua:	L. P. Chitta, D. Calchetti, J. Hirzberger, G. Valori, E. R. Priest, S. K. Solanki, D. Berghmans, C. Verbeeck, E. Kraaikamp, K. Albert, T. Appourchaux, F. J. Bailén, L. R. Bellot Rubio, J. Blanco Rodríguez, A. Feller, A. Gandorfer, L. Gizon, A. Lagg, A. Moreno Vacas, D. Orozco Suárez, J. Schou, U. Schühle, J. Sinjan, H. Strecker, R. Volkmer, J. Woch, X. Li, T. Oba, A. Ulyanov
Hōputu:	Artigo
Reo:	Inglês
I whakaputaina:	IOP Publishing 2025-01-01
Rangatū:	The Astrophysical Journal Letters
Ngā marau:	Solar magnetic fields Supergranulation Solar chromosphere Solar meridional circulation
Urunga tuihono:	https://doi.org/10.3847/2041-8213/ae10a3
Ngā Tūtohu:	Tāpirihia he Tūtohu Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!

Supergranulation and Poleward Migration of the Magnetic Field at High Latitudes of the Sun

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