“…Previously, electrically small antenna (ESA) designs capable of sufficiently high power and tuning range to enable transportable ionospheric heating were described (Esser et al, ), (Esser et al, ), (Esser et al, ), based on the 3‐D EZ magnetically (inductively) coupled ESA design introduced in Erentock and Ziolkowski () with a 100‐MHz design also presented (Lin et al, ). These designs are inherently matched to a 50 Ω feed line, requiring no additional matching networks, such as the networks used by the High‐Frequency Active Auroral Research Program (HAARP) (Jacobson et al, ); thereby, power capability is not limited by such external networks.…”