2006
DOI: 10.1016/j.asr.2004.12.008
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Artificial field-aligned irregularities in the nightside auroral ionosphere

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Cited by 19 publications
(22 citation statements)
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“…The same result was obtained by Blagoveshchenskaya et al (1999Blagoveshchenskaya et al ( , 2006a when strong heaterinduced striations were observed in the auroral E-region with bi-static HF radio scatter. Striations have also been observed from Tromsø HF heating experiments in the night-side Fregion of the auroral ionosphere when foF2 drops below the heater frequency by up to 0.5 MHz (Blagoveshchenskaya et al, 2006b). In all these studies the condition of the auroral ionosphere was monitored by ionosonde data.…”
Section: Introductionmentioning
confidence: 96%
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“…The same result was obtained by Blagoveshchenskaya et al (1999Blagoveshchenskaya et al ( , 2006a when strong heaterinduced striations were observed in the auroral E-region with bi-static HF radio scatter. Striations have also been observed from Tromsø HF heating experiments in the night-side Fregion of the auroral ionosphere when foF2 drops below the heater frequency by up to 0.5 MHz (Blagoveshchenskaya et al, 2006b). In all these studies the condition of the auroral ionosphere was monitored by ionosonde data.…”
Section: Introductionmentioning
confidence: 96%
“…The excitation of artificial small-scale field-aligned irregularities or striations (Minkoff et al, 1974;Djuth et al, 1985;Blagoveshchenskaya et al, 1999Blagoveshchenskaya et al, , 2006b), HF-induced electron heating (Rietveld et al, 2003) and airglow (Brandstrom et al, 1999;Pedersen and Carlson, 2001;Kosch et al, 2002), anomalous absorption (Robinson, 1989) and other phenomena occur at the upper hybrid resonance altitude in HF heating experiments when O-mode polarized HF pump waves reach the ionospheric reflection height. An O-mode HF pump wave couples through striations into electrostatic (upper hybrid) waves at the upper-hybrid resonance altitude, which is below the reflection height of the heating wave.…”
Section: Introductionmentioning
confidence: 99%
“…We report experimental results related to probing medium-scale traveling ionospheric disturbances using HF-induced scatter targets at mid-and high latitudes. With bi-static HF Doppler scatter, the AFAIs are being studied at middle (Blagoveshchenskaya and Troshichev, 1996;Yampolski et al, 1997;Blagoveshchenskaya et al, 1998a) and high latitudes (Blagoveshchenskaya et al, 1998b(Blagoveshchenskaya et al, , 1999(Blagoveshchenskaya et al, , 2006Rietveld et al, 2003). The proposed observational technique was used for the first time to identify the medium-scale TIDs.…”
Section: Introductionmentioning
confidence: 99%
“…The resulting expected deepening of the duct locally moves the upper hybrid resonance height upward. Since in the L-mode the wave electric field is perpendicular to B 0 at higher plasma densities than in the O-mode, the L-mode facilitates excitation of upper hybrid phenomena localized in the density depletions of small-scale striations (Vas'kov and Gurevich, 1976;Dysthe et al, 1982;Gurevich et al, 1995;Istomin and Leyser, 1997) and associated anomalous absorption deeper into the plasma (at higher ambient plasma densities) and in a wider altitude range than for pure Omode propagation. The duct, so to speak, tells the pump wave where to propagate and the pump wave tells the duct where to deepen, which may lead to self-focusing in magnetic zenith.…”
Section: Discussionmentioning
confidence: 99%
“…Experiments with the high-latitude EISCAT (European Incoherent SCATter association) high-power HF facility (named Heating) in northern Norway and the HAARP (High frequency Active Auroral Research Program) HF facility in Alaska, USA, show intensified optical emissions (Kosch et al, 2000;Pedersen and Carlson, 2001;Rietveld et al, 2003) and selffocusing (Gustavsson et al, 2001;Kosch et al, 2007) in magnetic zenith. Further, electron temperature enhancements are the largest when pumping near magnetic zenith (Rietveld et al, 2003;Honary et al, 2011) and pump-excited geomagnetic field-aligned density striations give the strongest HF-radar backscatter, as observed in experiments with EIS-CAT Heating (Rietveld et al, 2003;Blagoveshchenskaya et al, 2006), and the mid-latitude Sura HF facility in Russia (Tereshchenko et al, 2004). The question is, what causes the strong plasma response in magnetic zenith?…”
Section: Introductionmentioning
confidence: 99%