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http://nopr.niscpr.res.in/handle/123456789/25875Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Rahman, M M | - |
| dc.date.accessioned | 2014-01-20T07:25:08Z | - |
| dc.date.available | 2014-01-20T07:25:08Z | - |
| dc.date.issued | 2001-06 | - |
| dc.identifier.issn | 0975-105X (Online); 0367-8393 (Print) | - |
| dc.identifier.uri | http://hdl.handle.net/123456789/25875 | - |
| dc.description | 127-129 | en_US |
| dc.description.abstract | The extra-terrestrial solar radiation Ho mainly depends on different parameters (δ, ωs,ϕ, Eo), where the solar declination angle δ and the eccentricity correction factor Eo are only the variable quantities in a particular site. The present work compares the different forms of δ and Eo and recommends one that is most appropriate to assess the value of Ho as well as the solar radiations. | 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.30(3) [June 2001] | en_US |
| dc.title | A better method for computing Ho appearing in the correlations of solar radiation estimates | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | IJRSP Vol.30(3) [June 2001] | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| IJRSP 30(3) 127-129.pdf | 594.23 kB | Adobe PDF | View/Open |
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