000007756 001__ 7756
000007756 005__ 20260108085510.0
000007756 037__ $$aOUTRART-2026-0003
000007756 100__ $$aChitta, L. P. 
000007756 245__ $$aPicoflare jets in the coronal holes and their link to the solar wind 
000007756 260__ $$c2025
000007756 520__ $$aCharged particles continuously stream out from the million Kelvin hot corona as the solar wind. High-resolution extreme ultraviolet observations from the Solar Orbiter are providing new insights into the generation process of the solar wind. In particular, high-speed jets are observed to be widespread in darker interiors of coronal holes where the magnetic field stretches into the heliosphere. These jets could be the intermittent but prevalent seeds of the solar wind. Here we present our latest study from the Solar Orbiter mission and discuss their implications for the magnetic processes governing the solar wind origin.
000007756 594__ $$aSTCE
000007756 6531_ $$aSolar Orbiter
000007756 6531_ $$aEUI
000007756 6531_ $$ajets
000007756 6531_ $$asolar wind
000007756 700__ $$aHuang, Z. 
000007756 700__ $$aD’Amicis, R. 
000007756 700__ $$aCalchetti, D.
000007756 700__ $$aZhukov, A. N.  
000007756 700__ $$aKraaikamp, E. 
000007756 700__ $$aVerbeeck, C. 
000007756 700__ $$aAznar Cuadrado, R.  
000007756 700__ $$aHirzberger, J.  
000007756 700__ $$aBerghmans, D.  
000007756 700__ $$aHorbury, T. S.  
000007756 700__ $$aSolanki, S. K.  
000007756 700__ $$aOwen, C. J. 
000007756 700__ $$aHarra, L. 
000007756 700__ $$aPeter, H.  
000007756 700__ $$aSchühle, U. 
000007756 700__ $$aTeriaca, L.  
000007756 700__ $$aLouarn, P.  
000007756 700__ $$aLivi, S. 
000007756 700__ $$aGiunta, A. S.  
000007756 700__ $$aHassler, D. M.  
000007756 700__ $$aWang, Y.-M. 
000007756 773__ $$n#56$$pSolar Orbiter Science Nugget$$v02/04/2025$$y2025
000007756 8560_ $$fdavid.berghmans@ksb-orb.be
000007756 85642 $$ahttps://www.cosmos.esa.int/web/solar-orbiter/-/science-nugget-picoflare-jets-in-the-coronal-holes-and-their-link-to-the-solar-wind
000007756 980__ $$aOUTRART