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http://nopr.niscpr.res.in/handle/123456789/37535Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Manchanda, R K | - |
| dc.date.accessioned | 2016-11-25T04:26:05Z | - |
| dc.date.available | 2016-11-25T04:26:05Z | - |
| dc.date.issued | 1976-03 | - |
| dc.identifier.issn | 0975-105X (Online); 0367-8393 (Print) | - |
| dc.identifier.uri | http://nopr.niscair.res.in/handle/123456789/37535 | - |
| dc.description | 13-15 | en_US |
| dc.description.abstract | Monte-Carlo technique is used to compute the growth curve of the primary X-rays, incident on the top of the atmosphere. The calculations take into account the photo-electric attenuation and the multiple Compton scattering. From the comparison of the observed features and the calculated growth curves or primary X-rays, the functional form of the secondary X-rays is derived. These values are compared with the secondary X-rays deduced by log-linear and log-log extrapolation procedures. Effect of these computations on the diffuse back-ground spectrum is evaluated. | 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 | Functional Form of the Growth Curves for Balloon-borne X-ray Telescopes | 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) 13-15.pdf | 265.18 kB | Adobe PDF | View/Open |
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