Solar wind rotation rate and shear at coronal hole boundaries - Possible consequences for magnetic field inversionsR. F. Pinto, N. Poirier, A. P. Rouillard, A. Kouloumvakos, L. Griton, N. Fargette, R. Kieokaew, B. Lavraud and A. S. BrunA&A, 653 (2021) A92DOI: https://doi.org/10.1051/0004-6361/202040180