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http://nopr.niscpr.res.in/handle/123456789/36372Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Ghosh, S N | - |
| dc.contributor.author | Midya, S K | - |
| dc.date.accessioned | 2016-10-27T11:15:04Z | - |
| dc.date.available | 2016-10-27T11:15:04Z | - |
| dc.date.issued | 1989-02 | - |
| dc.identifier.issn | 0975-105X (Online); 0367-8393 (Print) | - |
| dc.identifier.uri | http://nopr.niscair.res.in/handle/123456789/36372 | - |
| dc.description | 33-35 | en_US |
| dc.description.abstract | Following Barth’s mechanism a theoretical curve of 5577 Å line emission at night with height is presented. An empirical relation between emission and height is then obtained from it. Experimental curve obtained by Kulkarni P V [J Geophys Res (USA), 81 (1976) 3740] gives intensity which agrees with that obtained from the curve of Barth’s mechanism. The intensity of 5577 Å line comes out to be 156 Rayleigh from the Chapman’s curve vis-à-vis 210 Rayleigh from the Barth’s mechanism, the latter value agrees with the accepted value 200 Rayleigh. | 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 | 5577 Å Night Airglow Emission from Barth’s and Chapman’s Mechanisms | 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) 33-35.pdf | 134.4 kB | Adobe PDF | View/Open |
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200 Rayleigh.