Author:
Paschmann G.,Sckopke N.,Vaith H.,Quinn J. M.,Bauer O. H.,Baumjohann W.,Fillius W.,Haerendel G.,Kerr S. S.,Kletzing C. A.,Lynch K.,McIlwain C. E.,Torbert R. B.,Whipple E. C.
Abstract
Abstract. We present the first electron time-of-flight measurements obtained with the Electron Drift Instrument (EDI) on Equator-S. These measurements are made possible by amplitude-modulation and coding of the emitted electron beams and correlation with the signal from the returning electrons. The purpose of the time-of-flight measurements is twofold. First, they provide the drift velocity, and thus the electric field, when the distance the electrons drift in a gyro period becomes sufficiently large. Second, they provide the gyro time of the electrons emitted by the instrument, and thus the magnitude of the ambient magnetic field, allowing in-flight calibration of the flux-gate magnetometer with high precision. Results of both applications are discussed.Key words. Magnetospheric physics (electric fields; plasma convection; instruments and techniques)
Subject
Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Geology,Astronomy and Astrophysics
Cited by
6 articles.
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