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http://nopr.niscpr.res.in/handle/123456789/36443Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Lokandaham, B. | - |
| dc.contributor.author | Yellaiah, G | - |
| dc.contributor.author | Tyagi, T R | - |
| dc.contributor.author | Singh, Lakha | - |
| dc.date.accessioned | 2016-10-28T11:17:25Z | - |
| dc.date.available | 2016-10-28T11:17:25Z | - |
| dc.date.issued | 1988-06 | - |
| dc.identifier.issn | 0975-105X (Online); 0367-8393 (Print) | - |
| dc.identifier.uri | http://nopr.niscair.res.in/handle/123456789/36443 | - |
| dc.description | 114-116 | en_US |
| dc.description.abstract | The enhancement in TEC during the periods of some mail meteor showers is estimated utilizing the 136 MHz ETS-II Faraday rotation measurements carried out at Hyderabad (1.5ᵒN, 78.3ᵒE), a low latitude station. The Geminid meteor shower produced maximum enhancement (about 40 per cent) compared to other showers. These observations show that there is a definite contribution to TEC of the ionosphere due the ionization produced by the meteors during the shower period. | 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.17(3) [June 1988] | en_US |
| dc.title | TEC Enhancement during Periods of Major Meteor Showers | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | IJRSP Vol.17(3) [June 1988] | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| IJRSP 17(3) 114-116.pdf | 235.56 kB | Adobe PDF | View/Open |
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