Abstract:First, an approximate evaluation is made of the ELF/VLF dipole moment of the polar electrojet antenna established by ionospheric heating via the use of powerful HF waves amplitude modulated with frequencies in the ELF/VLF range. Then, the theory of reciprocity is used to determine the magnitude of the ELF/VLF waveguide excitation produced by such a dipole immersed in the ionosphere. Propagation under a series of ionospheres ranging from quiet auroral nightime to disturbed auroral daytime is considered. contras… Show more
“…The first one, which is in the altitude range 60 km-85 km, is caused by the increasing of electron temperature, and the other, which is in the altitude range 90 km-95 km, is aroused by the increase of electron density. In Figure 5(a), the jumping phase near 77 km cancels out part of Pedersen currents; therefore, the Pedersen currents decrease, and this result is similar to the conclusion in reference [20].…”
Section: Numerical Results Analysis and Discussionsupporting
Abstract-Based on the theory of ionospheric heating, with the self-consistent model in the low ionosphere, the Extremely-Low-Frequency (ELF) and Very-Low-Frequency (VLF) waves generated by modulated beat-wave ionospheric heating are analyzed theoretically. In the consideration of the stratified ionosphere, the magnetic fields generated by the equivalent ELF/VLF dipole source above the sea surface are studied by using the quasi-longitudinal approximation method. Taking the high latitude regions as an example, the variations of the electron temperature, the increments of Pedersen and Hall conductivities and the changing of the oscillating current density with the modulation frequency in beatwave heating are numerically discussed. The distribution of the magnetic fields is presented. It turns out that in high latitude regions, the efficiency of rectangular wave modulated heating in generating ELF/VLF wave is higher than that of modulated beat-wave heating, and the order of magnitude of the magnetic fields received above the sea surface is 10 −7 A/m in beat-wave modulation.
“…The first one, which is in the altitude range 60 km-85 km, is caused by the increasing of electron temperature, and the other, which is in the altitude range 90 km-95 km, is aroused by the increase of electron density. In Figure 5(a), the jumping phase near 77 km cancels out part of Pedersen currents; therefore, the Pedersen currents decrease, and this result is similar to the conclusion in reference [20].…”
Section: Numerical Results Analysis and Discussionsupporting
Abstract-Based on the theory of ionospheric heating, with the self-consistent model in the low ionosphere, the Extremely-Low-Frequency (ELF) and Very-Low-Frequency (VLF) waves generated by modulated beat-wave ionospheric heating are analyzed theoretically. In the consideration of the stratified ionosphere, the magnetic fields generated by the equivalent ELF/VLF dipole source above the sea surface are studied by using the quasi-longitudinal approximation method. Taking the high latitude regions as an example, the variations of the electron temperature, the increments of Pedersen and Hall conductivities and the changing of the oscillating current density with the modulation frequency in beatwave heating are numerically discussed. The distribution of the magnetic fields is presented. It turns out that in high latitude regions, the efficiency of rectangular wave modulated heating in generating ELF/VLF wave is higher than that of modulated beat-wave heating, and the order of magnitude of the magnetic fields received above the sea surface is 10 −7 A/m in beat-wave modulation.
“…The six curves in each panel indicate how the normalized ELF response varies with the duty cycle of the pulse waveform for ionospheric cooling time constants varying from 0.1s h to 30s h . This range of time constants is similar to that calculated for the Hall current in the Dregion of the ionosphere (Rietveld et al, 1986) and the Hall current is normally regarded as the dominant current producing the ELF/VLF magnetic ®eld signatures at the Earth's surface (Barr and Stubbe, 1984b). The response axes in Fig.…”
Section: Rationale For Modulation Waveformsupporting
confidence: 54%
“…14 together with below by powerful HF waves modulated at ELF (3 kHz). They computed the time constants for the Hall current in preference to the Pedersen current as the Hall current had been shown to produce the dominant integrated dipole moment in studies used to determine the eective excitation of the Earth-ionosphere-waveguide by ELF current sources in the ionosphere produced by amplitude modulated HF heating (Barr and Stubbe, 1984b). In Fig.…”
Abstract. This paper describes the results of a preliminary study to determine the eective heating and cooling time constants of ionospheric currents in a simulated modulated HF heating,`beam painting' con®guration. It has been found that even and odd harmonics of the fundamental ELF wave used to amplitude modulate the HF heater are sourced from dierent regions of the ionosphere which support signi®cantly dierent heating and cooling time constants. The fundamental frequency and its odd harmonics are sourced in a region of the ionosphere where the heating and cooling time constants are about equal. The even harmonics on the other hand are sourced from regions of the ionosphere characterised by ratios of cooling to heating time constant greater than ten. It is thought that the even harmonics are sourced in the lower ionosphere (around 65 km) where the currents are much smaller than at the higher altitudes around 78 km where the currents at the fundamental frequency and odd harmonics maximise.
“…All the trajectories were in the south-to-north direction. Barr et al, 1985Barr et al, , 1986Rietveld et al, 1989). Also, Getmantsev et al (1974) performed the first ground-based observation of radiation at combination frequencies under HF heating, while Kotik and Trakhtengerts (1975) provided a theoretical treatment of this effect.…”
Abstract.It is now well known that amplitude modulated HF transmissions into the ionosphere can be used to generate ELF/VLF signals using the so-called "electrojet antenna". Although most observations of the generated ELF/VLF signals have been made on the ground, several low and highaltitude satellite observations have also been reported (James et al., 1990). One of the important unknowns in the physics of ELF/VLF wave generation by ionospheric heating is the volume of the magnetosphere illuminated by the ELF/VLF waves. In an attempt to investigate this question further, ground-satellite conjunction experiments have recently been conducted using the four Cluster satellites and the HF heater of the High-Frequency Active Auroral Research Program (HAARP) facility in Gakona, Alaska. Being located on largely closed field lines at L≈4.9, HAARP is currently also being used for ground-to-ground type of ELF/VLF waveinjection experiments, and will be increasingly used for this purpose as it is now being upgraded for higher power operation. In this paper, we describe the HAARP installation and present recent results of the HAARP-Cluster experiments. We give an overview of the detected ELF/VLF signals at Cluster, and a possible explanation of the spectral signature detected, as well as the determination of the location of the point of injection of the HAARP ELF/VLF signals into the magnetosphere using ray tracing.
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