7756 20260108085510.0 OUTRART-2026-0003 Chitta, L. P. Picoflare jets in the coronal holes and their link to the solar wind 2025 Charged particles continuously stream out from the million Kelvin hot corona as the solar wind. High-resolution extreme ultraviolet observations from the Solar Orbiter are providing new insights into the generation process of the solar wind. In particular, high-speed jets are observed to be widespread in darker interiors of coronal holes where the magnetic field stretches into the heliosphere. These jets could be the intermittent but prevalent seeds of the solar wind. Here we present our latest study from the Solar Orbiter mission and discuss their implications for the magnetic processes governing the solar wind origin. STCE Solar Orbiter EUI jets solar wind Huang, Z. D’Amicis, R. Calchetti, D. Zhukov, A. N. Kraaikamp, E. Verbeeck, C. Aznar Cuadrado, R. Hirzberger, J. Berghmans, D. Horbury, T. S. Solanki, S. K. Owen, C. J. Harra, L. Peter, H. Schühle, U. Teriaca, L. Louarn, P. Livi, S. Giunta, A. S. Hassler, D. M. Wang, Y.-M. Solar Orbiter Science Nugget 02/04/2025 2025 #56 david.berghmans@ksb-orb.be https://www.cosmos.esa.int/web/solar-orbiter/-/science-nugget-picoflare-jets-in-the-coronal-holes-and-their-link-to-the-solar-wind OUTRART