Comparison of Electric Dipole and Magnetic Loop Antennas for Whistler Generation in the Inner Magnetosphere
POSTER
Abstract
There has been much interest over the years in the use of very low frequency (VLF) whistlers in the inner magnetosphere for remediation of trapped MeV electrons in the Van Allen belts. In preparation for future satellite-borne experiments, it is essential to differentiate the best antenna design to generate whistler modes in the magnetosphere. The two simplest and most studied antennas are an electric dipole and a magnetic loop antenna. It is well known that a loop antenna is much better at radiating whistlers than a dipole, but a dipole is easier to deploy in space especially when antenna dimensions have to be large for VLF wave generation. This study compares the performance between the two antennas which are modeled in a cold magnetoplasma. The radiation resistance, the efficiency of whistler generation, radiation patterns, and effective antenna dimensions are compared for any orientation of both antennas with respect to the magnetic field and over a range of altitudes.
Authors
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Kevin Shipman
Los Alamos National Laboratory
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Patrick Colestock
Los Alamos National Laboratory
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Quinn Marksteiner
Los Alamos National Laboratory
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Gian Luca Delzanno
LANL, Los Alamos National Laboratory
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Bruce Carlsten
LANL, Los Alamos National Laboratory
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Mark Gilmore
University of New Mexico