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<p><strong>Abstract.</strong> Multi-year (1995&ndash;2013) velocity data collected by the Super Dual Auroral Network (SuperDARN) HF radars are considered to investigate seasonal and solar cycle variations of the convection reversal boundary (CRB) location for interplanetary magnetic field (IMF) <i>B</i><sub><i>z</i></sub> &lt; 0. By considering monthly data sets we show that the CRB is at higher latitudes in summer between 1995 and 2007. The poleward shifts are on the order ofdoi:10.5194/angeo-34-227-2016 fatcat:27jvtojlifdsdhaqlmohp5mhgu