Outer heliospheric radio emissions. I: Constraints on emission processes and the source region
In: JGR. Journal of geophysical research. Part A, Space physics, Jg. 97 (1992), Heft 5, S. 6235-6244
academicJournal
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Zugriff:
The Voyager 1 and 2 spacecraft observed low-frequency radio emissions near 2 and 3 kHz during the interval 1983-1987 while at heliocentric distances from 15 to 27 AU and 11 to 20 AU, respectively. We consider the detailed theoretical and observational requirements for this radiation to be produced near multiples of the plasma frequency fp by nonlinear, weak turbulence, wave-wave processes involving electrostatic Langmuir waves. Constraints on the emission processes and source characteristics are discussed.
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Outer heliospheric radio emissions. I: Constraints on emission processes and the source region
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Autor/in / Beteiligte Person: | CAIRNS, I. H ; GURNETT, D. A |
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Zeitschrift: | JGR. Journal of geophysical research. Part A, Space physics, Jg. 97 (1992), Heft 5, S. 6235-6244 |
Veröffentlichung: | Washington, DC: American Geophysical Union, 1992 |
Medientyp: | academicJournal |
Umfang: | print, 1 p |
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