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http://nopr.niscpr.res.in/handle/123456789/25888Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Lalmani | - |
| dc.contributor.author | Kumar, Rajou | - |
| dc.contributor.author | Singh, Rajesh | - |
| dc.contributor.author | Singh, Birbal | - |
| dc.date.accessioned | 2014-01-20T08:58:31Z | - |
| dc.date.available | 2014-01-20T08:58:31Z | - |
| dc.date.issued | 2001-08 | - |
| dc.identifier.issn | 0975-105X (Online); 0367-8393 (Print) | - |
| dc.identifier.uri | http://hdl.handle.net/123456789/25888 | - |
| dc.description | 214-216 | en_US |
| dc.description.abstract | First observations on the relationship between whistlers and periodic very low frequency (VLF) emissions observed at low latitude ground station Jammu (geomagn. lat., 22° 26' N; L = 1.17) are presented. The results have been discussed in the present paper. To explain the results it is proposed that the periodic VLF emissions are generated near the equatorial region at L ~ 1.2 as a result of interaction between trapped energetic particles and one-hop whistlers under cyclotron resonance mechanism and propagated to the ground station Jammu in nonducted mode of whistler propagation. | 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.30(4) [August 2001] | en_US |
| dc.title | Characteristics of the observed low latitude very low frequency emission periods and whistler-mode group delays at Jammu | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | IJRSP Vol.30(4) [August 2001] | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| IJRSP 30(4) 214-216.pdf | 569.19 kB | Adobe PDF | View/Open |
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