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Quasi-thermal Noise Spectra Measured by a Dipole Antenna in the Upper Hybrid frequency band
Authors:Yury V Chugunov  Anna Yu Kazarova  Eugene A Mareev  Michel Moncuquet  Karine Issautier  Nicole Meyer-Vernet
Institution:(1) Institute of Applied Physics RAS, Nizhny Novgorod, Russia;(2) DESPA, Observatoire de Paris, Meudon, France
Abstract:Quasi-thermal noise (QTN) spectroscopy is one of the most effective tools for in situ diagnostics in space plasmas (Meyer-Vernet et al., 1998; Meyer-Vernet and Perche, 1989; Chugunov and Trakhtengerts, 1978). This method produces routine measurements of the bulk electron density and temperature; recently it has been extended to measure the ion bulk speed. Among the advantages of the method its immunity to spacecraft potential and photoelectron perturbations should be noted. Quasi-thermal noise spectroscopy is used particularly on Ulysses and Wind. However for the interpretation of QTN data the calculation of the noise voltage induced on antennas under different conditions is necessary. This question is especially complicated and so far insufficiently studied in magnetized plasmas. In the present paper we calculate the spectrum of the noise voltage induced on a dipole antenna in the upper hybrid frequency range. The computations are adapted to the interpretation of data acquired on the Ulysses and Wind spacecraft. This revised version was published online in July 2006 with corrections to the Cover Date.
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