Please use this identifier to cite or link to this item:
http://nopr.niscpr.res.in/handle/123456789/37559Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Chiplonkar, M W | - |
| dc.date.accessioned | 2016-11-25T05:03:41Z | - |
| dc.date.available | 2016-11-25T05:03:41Z | - |
| dc.date.issued | 1976-03 | - |
| dc.identifier.issn | 0975-105X (Online); 0367-8393 (Print) | - |
| dc.identifier.uri | http://nopr.niscair.res.in/handle/123456789/37559 | - |
| dc.description | 92-94 | en_US |
| dc.description.abstract | The feasibility of detecting flare events on the back side of the sun from the observations of the radio emissions reflected by a suitably situated planet is pointed out. Rough quantitative estimates of signal strengths and signal-to-noise ratios are made to support the suggestion. The importance and uniqueness of such observations for prediction and solar flare data collection are stressed. | 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.05(1) [March 1976] | en_US |
| dc.title | Detection of Flares on the Back Side of the Sun | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | IJRSP Vol.05(1) [March 1976] | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| IJRSP 5(1) 92-94.pdf | 256.45 kB | Adobe PDF | View/Open |
Items in NOPR are protected by copyright, with all rights reserved, unless otherwise indicated.