2019
DOI: 10.1134/s0016793219060045
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Characterization of Artificial, Small-Scale, Ionospheric Irregularities in the High-Latitude F Region Induced by High-Power, High-Frequency Radio Waves of Extraordinary Polarization

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Cited by 11 publications
(15 citation statements)
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“…It is important to note that at lower heater frequencies the excitation threshold of the X-mode FAIs is much less. Blagoveshchenskaya et al (2019) found that during the EISCAT X-mode power stepping experiment at a heater frequency f H = 4.040 MHz the threshold of ERP for the FAI excitation was about 45 MW. It is also evident from Figure 8 that similar to the experiments on 3 November 2013 and 26 October 2013 described above, the X-mode HFPLs and HFILs were much stronger as compared to the O-mode ones.…”
Section: 1029/2020ja028203mentioning
confidence: 99%
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“…It is important to note that at lower heater frequencies the excitation threshold of the X-mode FAIs is much less. Blagoveshchenskaya et al (2019) found that during the EISCAT X-mode power stepping experiment at a heater frequency f H = 4.040 MHz the threshold of ERP for the FAI excitation was about 45 MW. It is also evident from Figure 8 that similar to the experiments on 3 November 2013 and 26 October 2013 described above, the X-mode HFPLs and HFILs were much stronger as compared to the O-mode ones.…”
Section: 1029/2020ja028203mentioning
confidence: 99%
“…The comparable analysis of the HFPL, HFIL, and FAI behaviors on 3 November 2013 (f H = 6.2 MHz) and 26 October 2013 (f H = 6.96 MHz) has revealed that FAIs play a key role in the excitation of a nonresonant PDI under X-mode HF pumping. The generation conditions and features of the X-mode FAIs excited in the high-latitude ionosphere F region at different pump frequencies from 4 to 8 MHz have been intensively investigated from numerous EISCAT heating experiments by Blagoveshchenskaya et al (2011Blagoveshchenskaya et al ( , 2013Blagoveshchenskaya et al ( , 2015Blagoveshchenskaya et al ( , 2019. It was found that the X-mode FAI excitation occurred in two steps.…”
Section: Journal Of Geophysical Research: Space Physicsmentioning
confidence: 99%
“…The analysis of the entire volume of the CUTLASS data clearly demonstrated that the features and behaviors of the O-mode and X-mode artifi cial fi eld-aligned irregularities radically diff ered. There was also a signifi cant diff erence in the decay times for X-mode artifi cial fi eld-aligned irregularities excited at high ( 5 [37]. As seen, the artifi cial fi eld-aligned irregularity growth and decay times signifi cantly diff ered for O-and X-mode HF pumping.…”
Section: Small-scale Artifi Cial Field-aligned Irregularities (Afais)mentioning
confidence: 78%
“…The behavior and properties of artifi cial fi eld-aligned irregularities excited by the O-mode HF pump waves are well known (see, for example, [13][14][15] and references therein). The main attention is paid to the recently discovered artifi cial fi eld-aligned irregularities induced by the X-mode HF pump waves and their comparison with the O-mode artifi cial fi eld-aligned irregularities [31][32][33][34][35][36][37].…”
Section: Small-scale Artifi Cial Field-aligned Irregularities (Afais)mentioning
confidence: 99%
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