Please use this identifier to cite or link to this item:
http://nopr.niscpr.res.in/handle/123456789/27002Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Shrivastava, Pankaj K. | - |
| dc.contributor.author | Singh, G. N. | - |
| dc.date.accessioned | 2014-02-27T05:20:53Z | - |
| dc.date.available | 2014-02-27T05:20:53Z | - |
| dc.date.issued | 2004-12 | - |
| dc.identifier.issn | 0975-2412 (Online); 0771-7706 (Print) | - |
| dc.identifier.uri | http://hdl.handle.net/123456789/27002 | - |
| dc.description | 261-262 | en_US |
| dc.description.abstract | Coronal Mass Ejections (CMEs) carry large amount of energy and mass into the interplanetary space. Recently CMEs are known as a main source of geomagnetic disturbances and changes in cosmic ray intensity. In this work, 55 halo CME events are selected for the period of 1996 to 2000 to derive their effects on cosmic ray intensity. It has been investigated that CMEs in association with sudden storm commencement (SSC) are found to be more effective in producing short-term transient decreases in cosmic ray intensity. | 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 | BVAAP Vol.12(2) [December 2004] | en_US |
| dc.title | Effect of Coronal Mass Ejections on cosmic ray intensity Variation | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | BVAAP Vol.12(2) [December 2004] | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| BVAAP 12(2) 261-262.pdf | 337.66 kB | Adobe PDF | View/Open |
Items in NOPR are protected by copyright, with all rights reserved, unless otherwise indicated.