“…Extremely low frequency (ELF, 3–3000 Hz) and very low frequency (VLF, 3–30 kHz) waves can be generated by modulated high frequency (HF, 3–30 MHz) heating of the D ‐region ionosphere (∼60–100 km altitude) in the presence of naturally forming electric currents, such as the auroral electrojet [e.g., Getmantsev et al , 1974; Stubbe et al , 1982; Papadopoulos et al , 2003; Moore et al , 2007; Cohen et al , 2010]. The magnitude of ELF/VLF waves generated in this manner are dependent upon the ambient ionospheric conditions, such as the electron density and the electron temperature [e.g., Tomko et al , 1980; Stubbe et al , 1982; Barr and Stubbe , 1984; James et al , 1984; Rietveld and Stubbe , 1987; Papadopoulos et al , 1990; Barr and Stubbe , 1991a, 1991b; Moore , 2007; Cohen et al , 2010; Moore and Agrawal , 2011], as well as on the background geomagnetic conditions that drive the strength of the auroral electrojet [e.g., Stubbe et al , 1981; Rietveld et al , 1983; Papadopoulos et al , 2003; Payne , 2007; Jin et al , 2011]. Additionally, in an effort to understand the dynamics of high power radio wave heating of the ionosphere, a number of studies have investigated the dependence of the generated ELF/VLF signal strength on the HF transmission parameters, such as HF power, HF polarization, and modulation frequency [e.g., Ferraro et al , 1984; Barr and Stubbe , 1991a, 1991b; Villaseñor et al , 1996; Milikh et al , 1999; Moore et al , 2006; Fujimaru and Moore , 2011].…”