Please use this identifier to cite or link to this item:
http://nopr.niscpr.res.in/handle/123456789/36790Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Bharathi, G | - |
| dc.contributor.author | Raj, P Ernest | - |
| dc.contributor.author | Murthy, B Narasimha | - |
| dc.contributor.author | Jogulu, C | - |
| dc.date.accessioned | 2016-11-04T09:52:36Z | - |
| dc.date.available | 2016-11-04T09:52:36Z | - |
| dc.date.issued | 1982-06 | - |
| dc.identifier.issn | 0975-105X (Online); 0367-8393 (Print) | - |
| dc.identifier.uri | http://nopr.niscair.res.in/handle/123456789/36790 | - |
| dc.description | 96-99 | en_US |
| dc.description.abstract | True height electron density profiles are deduced from the ionograms taken at Gauhati (lat., 26°10'N; long., 91°45'E) on 16 Feb. 1980, a solar eclipse day. Constant electron density contours show a definite eclipse effect. A large increase in the height of the constant electron density levels, more pronounced at lower levels, is seen after first contact. The 'eclipse lag' is about 15 min at around 300 km. A long period wavelike oscillation observed at all electron density levels after the time of maximum obscuration could be eclipse generated. | 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.11(3) [June 1982] | en_US |
| dc.title | Electron Density Changes during Solar Eclipse of 16 Feb. 1980 at Gauhati | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | IJRSP Vol.11(3) [June 1982] | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| IJRSP 11(3) 96-99.pdf | 211.32 kB | Adobe PDF | View/Open |
Items in NOPR are protected by copyright, with all rights reserved, unless otherwise indicated.