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http://nopr.niscpr.res.in/handle/123456789/37622Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Singh, R N | - |
| dc.contributor.author | Singh, R P | - |
| dc.contributor.author | Rai, R S | - |
| dc.date.accessioned | 2016-11-25T10:17:57Z | - |
| dc.date.available | 2016-11-25T10:17:57Z | - |
| dc.date.issued | 1976-12 | - |
| dc.identifier.issn | 0975-105X (Online); 0367-8393 (Print) | - |
| dc.identifier.uri | http://nopr.niscair.res.in/handle/123456789/37622 | - |
| dc.description | 285-288 | en_US |
| dc.description.abstract | Using data from Pioneer-10 and Pioneer-11 for the Jovian magnetic field and energetic electron flux the problem of decametric radiation (DAM) has been studied. The total synchrotron power emitted from energetic electron flux in the Jovian atmosphere has been calculated and compared with the available measured data. The synchrotron mechanism of electromagnetic radiation is found to explain macroscopic features of the observed decametric emission. The modulation of DAM by Io has been discussed. | 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.05(4) [December 1976] | en_US |
| dc.title | Synchrotron Process as the Source of Decametric Radiation from Jupiter | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | IJRSP Vol.05(4) [December 1976] | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| IJRSP 5(4) 285-288.pdf | 1.05 MB | Adobe PDF | View/Open |
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