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http://nopr.niscpr.res.in/handle/123456789/36798Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Agrawal, S P | - |
| dc.contributor.author | Pathak, S P | - |
| dc.date.accessioned | 2016-11-04T10:13:41Z | - |
| dc.date.available | 2016-11-04T10:13:41Z | - |
| dc.date.issued | 1982-06 | - |
| dc.identifier.issn | 0975-105X (Online); 0367-8393 (Print) | - |
| dc.identifier.uri | http://nopr.niscair.res.in/handle/123456789/36798 | - |
| dc.description | 124-125 | en_US |
| dc.description.abstract | A comparison of the direction of the maximum flux of the second harmonic of the daily variation of cosmic ray intensity observed at Deep River (ɸ2), with the direction of the interplanetary magnetic field (ɸB), has been made for each day during 1973-75. The results show that, in general, the direction of ɸ2 is perpendicular to ɸB, which is in agreement with the earlier observations as well as with the theoretical predictions. | 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 | Direction of Semi-diurnal Anisotropy in Relation to Interplanetary Magnetic Fields | 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) 124-125.pdf | 147.73 kB | Adobe PDF | View/Open |
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