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http://nopr.niscpr.res.in/handle/123456789/25656Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Kane, R P | - |
| dc.date.accessioned | 2014-01-15T05:35:09Z | - |
| dc.date.available | 2014-01-15T05:35:09Z | - |
| dc.date.issued | 2005-06 | - |
| dc.identifier.issn | 0975-105X (Online); 0367-8393 (Print) | - |
| dc.identifier.uri | http://hdl.handle.net/123456789/25656 | - |
| dc.description | 171-174 | en_US |
| dc.description.abstract | A comparison of the variations of the cosmic ray neutron monitor intensities with variations of geomagnetic disturbance Dst and (number) densities N of interplanetary plasma observed near the Earth during June-August, 1979 and May 1999 (intervals when N was abnormally low) has been presented. It showed that cosmic ray variations were very loosely related to Dst variations (variations often out -of-phase by several days, and magnitudes not proportional) and had no relationship with plasma densities N (low or high). | en_US |
| dc.language.iso | en_US | en_US |
| dc.publisher | NISCAIR-CSIR, India | en_US |
| dc.relation.ispartof | 96.60.Vg; 96.40-z | en_US |
| dc.rights |  CC Attribution-Noncommercial-No Derivative Works 2.5 India | en_US |
| dc.source | IJRSP Vol.34(3) [June 2005] | en_US |
| dc.subject | Cosmic ray intensity | en_US |
| dc.subject | Solar wind | en_US |
| dc.subject | Geomagnetic indices | en_US |
| dc.subject | Interplanetary plasma density | en_US |
| dc.title | Cosmic ray variations during density extremes in solar wind | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | IJRSP Vol.34(3) [June 2005] | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| IJRSP 34(3) 171-174.pdf | 884.77 kB | Adobe PDF | View/Open |
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