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Electron plasma waves in the solar wind: AMPTE/IRM and UKS observations |
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| Institution: | 1. Max-Planck-Institut für hysik und Astrophysik, Institut für Extraterrestrische Physik, 8046 Garching, F.R.G.;2. School of Physics, The University of Sussex, Brighton, BN1 9QH, U.K.;3. Department of Physics, The University of Sheffield, Sheffield, S37RH, U.K.;4. Department of Physics and Astronomy, University of Iowa, Iowa City, IA 52242, U.S.A.;6. Space Sciences Division, University of Washington, Seattle, WA 98195, U.S.A.;5. The Aerospace Corporation, Los Angeles, CA 90009, U.S.A.;1. Department of Physics, Umeå University, SE-901 87 Umeå, Sweden;2. Department of Physics, Linköping University, SE-581 83 Linköping, Sweden |
| Abstract: | Selected events of plasma wave and electromagnetic emissions in the earth's electron fore-shock region have been studied. Strong emissions are observed in the plasma-wave band when the site of the satellite is magnetically connected to the bow shock. These emissions are generally highly fluctuating. Under certain conditions one observes electromagnetic radiation at the second harmonic produced locally. Electromagnetic emission generated at a position far away from the site of the spacecraft is occasionally detected giving rise to remote sensing of the bow shock. These emissions are related to energetic electron fluxes. |
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