“…One of the significant nonlocal effects of HF O-mode heating is the creation of O + ion outflows observed by the EISCAT UHF ISR, DMSP spacecraft, and HAARP Digisonde sky map technique [Rietveld et al, 2003;Milikh et al, 2010a;Blagoveshchenskaya et al, 2011;Kosch et al, 2010; 2014; Vartanyan et al, 2012] along with plasma density enhancements (artificial ducts) in the topside ionosphere measured onboard the DEMETER and DMSP spacecraft [Frolov et al, 2016;Milikh et al, 2008a;Rapoport et al, 2010;Markov et al, 2010;Vartanyan et al, 2012]. During satellite overflight experiments, the heating facility was usually turned on 10-20 min before the predicted satellite crossing the facility magnetic flux tube at the closest distance ΔRc from the center (MZ).…”