Editor's Foreword iii Acknowledgements iv
Incoherent Scatter spectra computed with a typical EISCAT observation of the ionosphere in the ~ 120- 500 km altitude range. The spectra shape varies with the altitude as function of the observed electron temperature and of the ion temperature and composition. The spectral power is scaled to the ele...
| Main Authors: | , |
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| Other Authors: | |
| Format: | Text |
| Language: | English |
| Published: |
1997
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| Online Access: | http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.622.8846 http://e7.eiscat.se/groups/Documentation/CourseMaterials/1995Cargese/Cargese book (previous school lectures).pdf |
| Summary: | Incoherent Scatter spectra computed with a typical EISCAT observation of the ionosphere in the ~ 120- 500 km altitude range. The spectra shape varies with the altitude as function of the observed electron temperature and of the ion temperature and composition. The spectral power is scaled to the electron density and the spectra are |
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