2013
DOI: 10.1002/jgra.50558
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100 days of ELF/VLF generation via HF heating with HAARP

Abstract: Extremely low frequency/very low frequency (ELF/VLF) radio waves are difficult to generate with conventional antennas. Ionospheric high frequency (HF) heating facilities generate ELF/VLF waves via modulated heating of the lower ionosphere. HF heating of the ionosphere changes the lower ionospheric conductivity, which in the presence of natural currents such as the auroral electrojet creates an antenna in the sky when heating is modulated at ELF/VLF frequencies. We present a summary of nearly 100 days of ELF/VL… Show more

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Cited by 37 publications
(26 citation statements)
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“…At the Arecibo Observatory in Puerto Rico and at the Jicamarca Observatory in Peru HF facilities were used to generate weak ELF signals with the equatorial electrojets [ Ferraro et al , ; Lunnen et al , ]. The European Incoherent Scatter facility located in Tromsø, Norway, the High Frequency Active Auroral Research Program (HAARP), and the Sura ionospheric heating facility in Russia have been extensively utilized for the modulation of auroral electrojets [ Stubbe et al , ; Barr and Stubbe , ; Moore et al , ; Fujimaru and Moore , ; Cohen et al , ; Gołkowski et al , ; Cohen and Golkowski , ; Kotik et al , ]. The two main modes of heating the ionosphere are called the ordinary mode ( O mode) and the extraordinary mode ( X mode).…”
Section: Introductionmentioning
confidence: 99%
“…At the Arecibo Observatory in Puerto Rico and at the Jicamarca Observatory in Peru HF facilities were used to generate weak ELF signals with the equatorial electrojets [ Ferraro et al , ; Lunnen et al , ]. The European Incoherent Scatter facility located in Tromsø, Norway, the High Frequency Active Auroral Research Program (HAARP), and the Sura ionospheric heating facility in Russia have been extensively utilized for the modulation of auroral electrojets [ Stubbe et al , ; Barr and Stubbe , ; Moore et al , ; Fujimaru and Moore , ; Cohen et al , ; Gołkowski et al , ; Cohen and Golkowski , ; Kotik et al , ]. The two main modes of heating the ionosphere are called the ordinary mode ( O mode) and the extraordinary mode ( X mode).…”
Section: Introductionmentioning
confidence: 99%
“…The first point of divergence concerns the natural generation mechanism of ELF magnetic field components presumably being the energy source of the Titan's SRs (Béghin, 2014), while the same process does not seem to occur naturally on Earth. However, the first successful attempt of artificial triggering of ELF emissions in the polar electrojet by High Frequency (HF) heating experiments (Mc Carrick et al, 1990) and furthermore performed quasi-routinely in VLF range (e.g., Cohen and Golkowski, 2013) bring a significant support to the model proposed here, though no experimental evidence is known to date about a natural ELF self-modulation of terrestrial electrojets. This is probably because the necessary increase of conductivity which is thought to exist naturally in Titan's ionopause for triggering the ion-acoustic instability and subsequently yielding the ELF modulation of the current, seems not occurring on Earth.…”
Section: Discussionmentioning
confidence: 62%
“…The physical process of ion-acoustic instability is basically the same as observed with the experiments of HF heating of the ionosphere in the Earth's Polar Regions in which the increase of Pedersen conductivity is triggered artificially (e.g. Stubbe and Koppa, 1977;Mc Carrick et al, 1990;Cohen and Golkowski, 2013), contrary to the natural process involved for Titan. The specific criterion for triggering the ion-acoustic instability is when the electron-ion drift velocity V drift exceeds the adiabatic ion-acoustic speed c s , which reads…”
Section: Interface Region Between Titan's Upper Atmosphere and Saturnmentioning
confidence: 88%
“…Observations at HAARP are $5-100 times stronger than at the Sura heating facility [19]. Cubic ELF and VLF wave generation is $30 dB weaker than auroral electrojet modulation in the 1-5 kHz range [29] and $10 dB weaker in the 16-20 kHz range [30]. It is also $3-6 dB weaker than the signals reported to be generated by the ionospheric current drive (ICD) mechanism [15], but cubic generation is strongest at higher frequencies (> 10 kHz), whereas the ICD is reported to be strongest at lower frequencies (< 100 Hz).…”
mentioning
confidence: 91%