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http://nopr.niscpr.res.in/handle/123456789/36369Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Ahmad, M M | - |
| dc.contributor.author | Lalmani | - |
| dc.contributor.author | Khosa, P N | - |
| dc.date.accessioned | 2016-10-27T11:11:57Z | - |
| dc.date.available | 2016-10-27T11:11:57Z | - |
| dc.date.issued | 1989-02 | - |
| dc.identifier.issn | 0975-105X (Online); 0367-8393 (Print) | - |
| dc.identifier.uri | http://nopr.niscair.res.in/handle/123456789/36369 | - |
| dc.description | 27-29 | en_US |
| dc.description.abstract | An attempt has been made to explain the various radio emissions of large frequency range observed in the Jupiter’s magnetosphere by the resonant interaction mechanism between the ion-cyclotron wave propagating along Jovian magnetic field lines and trapped fully ionize hydrogen plasma. The growth rate has been derived by the conservation of energy method for bi-Maxwellian distribution function in an anisotropic plasma. The variation of growth rate with propagation constant has been discussed, and the maximum growth rates for Jovian magnetospheric condition LJ=6 have been estimated for various values of the ratio of kinetic pressure to magnetic pressure and ion anisotropies. | 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.18(1) [February 1989] | en_US |
| dc.title | Electromagnetic Ion-cyclotron Mechanism in Jovian Magnetosphere | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | IJRSP Vol.18(1) [February 1989] | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| IJRSP 18(1) 27-29.pdf | 235.42 kB | Adobe PDF | View/Open |
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