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http://nopr.niscpr.res.in/handle/123456789/37833Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Ghosh, B. B. | - |
| dc.contributor.author | Malhotra, V. J. | - |
| dc.date.accessioned | 2016-11-29T08:45:30Z | - |
| dc.date.available | 2016-11-29T08:45:30Z | - |
| dc.date.issued | 1974-09 | - |
| dc.identifier.issn | 0975-105X (Online); 0367-8393 (Print) | - |
| dc.identifier.uri | http://nopr.niscair.res.in/handle/123456789/37833 | - |
| dc.description | 278-281 | en_US |
| dc.description.abstract | Results of analysis showing some effects on the field strengths of 164 kHz signal from Radio Tashkent (41° 25'N, 69° 12'E) recorded at Delhi (28° 35'N, 77° 05'E) due to meridian transits of a few stellar X-ray bodies at the midpoint (35° 04'N, 73° 24'E) of Tashkent-Delhi propagation path, have been reported. While the effects due to SCO-XR-1 and TAU-XR-1 show rather significant results in respect of their 'ion production rates' (cm-3 sec-1), those due to other stellar X-ray sources, Gx, 333 + 2.5 and CYG-XR-1 are small and rather unaccountable. For each star, records for a period of two months, during which respective meridian transits take place between 1900 and 2300 hrs 1ST (UT + 5 hrs), have been analyzed. | 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.03(3) [September 1974] | en_US |
| dc.title | Changes in 164 kHz Signal Field Strengths due to Stellar X-Ray Effects on D-Region Nighttime Ionization | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | IJRSP Vol.03(3) [September 1974] | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| IJRSP 3(3) 278-281.pdf | 942.8 kB | Adobe PDF | View/Open |
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