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http://nopr.niscpr.res.in/handle/123456789/36232Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Singh, V | - |
| dc.date.accessioned | 2016-10-26T09:15:59Z | - |
| dc.date.available | 2016-10-26T09:15:59Z | - |
| dc.date.issued | 1991-12 | - |
| dc.identifier.issn | 0975-105X (Online); 0367-8393 (Print) | - |
| dc.identifier.uri | http://nopr.niscair.res.in/handle/123456789/36232 | - |
| dc.description | 438-443 | en_US |
| dc.description.abstract | Using the plasma and field parameters corresponding to L=8, temporal growth rates of VLF waves have been computed for a non-Maxwellian electron distribution leads the generation of VLF chorus just below the one-half of the electron gyrofrequency and the presence of nonthermal drifted Maxwellian tail leads the instability below one-fourth of the electron gyrofrequency. The computed results are in good agreement with those reported by the Voyager 1 and 2 plasma wave experiments. | en_US |
| dc.language.iso | en_US | en_US |
| dc.publisher | NISCAIR-CSIR, India | en_US |
| dc.rights |  CC Attribution-Noncommercial-No Derivative Works 2.5 India | en_US |
| dc.source | IJRSP Vol.20(6) [December 1991] | en_US |
| dc.title | Generation of VLF hiss and chorus in Jupiter’s magnetosphere | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | IJRSP Vol.20(6) [December 1991] | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| IJRSP 20(6) 438-443.pdf | 1.24 MB | Adobe PDF | View/Open |
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