7700 20260105155453.0 10.3847/2041-8213/ae10a3 DOI SCART-2026-0008 Chitta, L. P. Supergranulation and Poleward Migration of the Magnetic Field at High Latitudes of the Sun 2025 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 from a high-latitude campaign of the Solar Orbiter spacecraft, which reveal spatial and temporal evolution of supergranular convective cells. The supergranular cells have spatial scales of 20–40 Mm. From 8 days of observations starting on 2025 March 16, our analysis shows that the magnetic network migrates poleward, on average, at high latitudes (above 60°), with speeds in the range of 10–20 m s−1, depending on the structures being tracked. These results shed light on the buildup of the polar magnetic field that is central to our understanding of the solar cycle and the heliospheric magnetic field. STCE Solar Orbiter EUI PHI high latitude Calchetti, D. Hirzberger, J. Valori, G. Priest, E. R. Solanki, S. K. Berghmans, D. Verbeeck, C. Kraaikamp, E. Albert, K. Appourchaux, T. Bailén, F. J. Bellot Rubio, L. R. Blanco Rodríguez, J. Feller, A. Gandorfer, A. Gizon, L. Lagg, A. Moreno Vacas, A. Orozco Suárez, D. Schou, J. Schühle, U. Sinjan, J. Strecker, H. Volkmer, R. Woch, J. Li, X. Oba, T. Ulyanov, A. The Astrophysical Journal Letters 993 2025 2, id.L45 david.berghmans@ksb-orb.be https://arxiv.org/abs/2509.26586 https://iopscience.iop.org/article/10.3847/2041-8213/ae10a3 published in REFERD