www.ann-geophys.net/23/101/2005/ doi:10.5194/angeo-23-101-2005 © European Geosciences Union 2005 Pulsed energy storage antennas for ionospheric modification 1UCLA Plasma Physics Lab., Los Angeles, CA 90095, USA 2HIPAS Observatory Two Rivers, AK 99712, USA *now retired from UCLA Abstract. Interesting, "new", very high peak-power pulsed radio frequency (RF) antennas have been assembled at the HIPAS Observatory (Alaska, USA) and also at the University of California at Los Angeles (UCLA, USA); namely, a pair of quarter wavelength (λ/4) long cylindrical conductors separated by a high voltage spark gap. Such a combination can radiate multi-megawatt RF pulses whenever the spark gap fires. The antenna at HIPAS is 53m long (λ/2) with a central pressurized SF6 spark gap. It is mounted 5 meters (λ/21) above a ground plane. It radiates at 2.85MHz. The two antenna halves are charged to ± high voltages by a Tesla coil. Spark gap voltages of 0.4 MV (at the instant of spark gap closure) give peak RF currents of ~1200A which correspond to ~14 MW peak total radiated power, or ~56 MW of Effective Radiated Power (ERP). The RF pulse train is initially square, decaying exponentially in time with Qs of ~50. Two similar but smaller 80-MHz antennas were assembled at UCLA to demonstrate their synchronization with a pulsed laser which fired the spark gaps in the two antennas simultanoeously. These experiments show that one can anticipate a pulsed array of laser synchronized antennas having a coherent Effective Radiated Power (ERP)>10GW. One can even reconsider a pulse array radiating at 1.43MHz which corresponds to the electron gyrofrequency in the Earth's magnetic field at ~200km altitude. These "new" pulsed high power antennas are hauntingly similar to the ones used originally by Hertz (1857-1894) during his (1886-1889) seminal verifications of Maxwell's (1864) theory of electrodynamics. Full Article (PDF, 978 KB) Citation: Wuerker, R. F., Chen, J., Beam, W., and Nichols, E.: Pulsed energy storage antennas for ionospheric modification, Ann. Geophys., 23, 101-107, doi:10.5194/angeo-23-101-2005, 2005. Bibtex EndNote Reference Manager XML |
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