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| Titel |
Radiation by energetic electrons accelerated by wave-particle interaction: a plausible mechanism for x-ray emission from the Venus mantle |
| VerfasserIn |
R. Bingham, K. B. Quest, V. D. Shapiro, B. J. Kellett |
| Medientyp |
Artikel
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| Sprache |
Englisch
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| ISSN |
0992-7689
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| Digitales Dokument |
URL |
| Erschienen |
In: Annales Geophysicae ; 26, no. 7 ; Nr. 26, no. 7 (2008-07-02), S.1829-1836 |
| Datensatznummer |
250016149
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| Publikation (Nr.) |
 copernicus.org/angeo-26-1829-2008.pdf |
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| Zusammenfassung |
| In this paper it is argued that recently observed x-ray emission
from non-magnetic planets (Dennerl et al., 2002) can be explained
as a combination of bremsstrahlung and line K-shell radiation
produced by the interaction of energetic electrons with the
neutral atmosphere. Numerical simulations show that the modified two stream
instability can generate energetic 100 eV electrons that are observed and these electrons can produce x-ray emission. |
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