2019
DOI: 10.1029/2019rs006857
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Three‐Dimensional Mapping of Lightning‐Produced Ionospheric Reflections

Abstract: The powerful high-frequency/very high frequency radio emissions that occur during lightning flashes can be used as a signal of opportunity to study the bottom side ionosphere. The lightning emission is bright, broad spectrum, and short in duration, providing an ideal signal of opportunity for making ionograms. This study continues previous work in Obenberger et al. (2018), where the direct line of sight signal from lightning can be cross correlated with megahertz frequency radio telescope observations to revea… Show more

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Cited by 6 publications
(5 citation statements)
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“…Detailed procedures on how such studies could be carried out are beyond the scope of the current paper. The TP technique may be complementary to the recently developed technique of using lightning as a HF source to produce ionograms (Malins et al, 2019; Obenberger et al, 2018).…”
Section: Possible Use Of Tps For Studying the Ionospherementioning
confidence: 99%
“…Detailed procedures on how such studies could be carried out are beyond the scope of the current paper. The TP technique may be complementary to the recently developed technique of using lightning as a HF source to produce ionograms (Malins et al, 2019; Obenberger et al, 2018).…”
Section: Possible Use Of Tps For Studying the Ionospherementioning
confidence: 99%
“…Data were collected at two distinct locations in New Mexico, LWA-1 and LWA-SV. One dataset was collected at the Long Wavelength Array (LWA)-SV station at the Sevilleta National Wildlife Refuge in central New Mexico [39]. The other set of data was obtained using the LWA-1 radio telescope array, which is positioned in northern New Mexico and has a diameter of 100 m. This radio telescope array is associated with the University Radio Observatory [40].…”
Section: Sdr Experimental Methodsmentioning
confidence: 99%
“…The LWA-SV and LWA-1 (University Radio Observatory) in central New Mexico captured radio wave frequencies from 3 MHz to 88 MHz, and each array consisted of 256 pairs of dipole-type antennas, while each pair of antennas had orthogonal polarizations on one stand. Antennas of the LWA-SV were arranged in a 110 m by 100 m north-south area distributed in about 100 m of aperture, as seen in Figure 2 [29]. Array geometry of the LWA-1 was within a 100 m (east-west) × 110 m (north-south) elliptical shape, as illustrated in Figure 3 [30].…”
Section: Lwa-sv and Lwa-1 Description Of New Mexico Experimentsmentioning
confidence: 99%