Source mechanism of Saturn narrowband emission
Narrowband emission (NB) is observed at Saturn centered near 5 kHz and 20 kHz and harmonics. This emission appears similar in many ways to Jovian kilometric narrowband emission observed at higher frequencies, and therefore may have a similar source mechanism. Source regions of NB near 20 kHz are...
| Main Authors: | , , , , |
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| Format: | Article |
| Language: | English |
| Published: |
Copernicus Publications
2010-04-01
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| Series: | Annales Geophysicae |
| Online Access: | https://www.ann-geophys.net/28/1013/2010/angeo-28-1013-2010.pdf |