Please use this identifier to cite or link to this item:
http://nopr.niscpr.res.in/handle/123456789/38096Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Srivastava, A. N. | - |
| dc.contributor.author | Srivastava, R. D. | - |
| dc.date.accessioned | 2016-12-02T09:13:14Z | - |
| dc.date.available | 2016-12-02T09:13:14Z | - |
| dc.date.issued | 1972-12 | - |
| dc.identifier.issn | 0975-105X (Online); 0367-8393 (Print) | - |
| dc.identifier.uri | http://nopr.niscair.res.in/handle/123456789/38096 | - |
| dc.description | 241-243 | en_US |
| dc.description.abstract | An analysis if the experimental results on absorption of ultraviolet radiation by atmospheric gases indicates that the absorption processes obey spin conservation rule. In the light of this, dayglow emissions of the Martian atmosphere are considered. It has been found that the red and green lines of OI and a number of spectral features of CO should be present and that their emission heights should be about 110-210 km from the surface of Mars. | 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.01(4) [December 1972] | en_US |
| dc.title | CO Emission in the Martian Dayglow | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | IJRSP Vol.01(4) [December 1972] | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| IJRSP 1(4) 241-243.pdf | 303.8 kB | Adobe PDF | View/Open |
Items in NOPR are protected by copyright, with all rights reserved, unless otherwise indicated.