Please use this identifier to cite or link to this item:
http://nopr.niscpr.res.in/handle/123456789/11930Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Kane, R P | - |
| dc.date.accessioned | 2011-06-07T10:23:21Z | - |
| dc.date.available | 2011-06-07T10:23:21Z | - |
| dc.date.issued | 2011-06 | - |
| dc.identifier.issn | 0975-105X (Online); 0367-8393 (Print) | - |
| dc.identifier.uri | http://hdl.handle.net/123456789/11930 | - |
| dc.description | 121-123 | en_US |
| dc.description.abstract | During 2007, the relationship of the variations in the daily values of sunspot number (Rz) and the 2800 MHz solar radio emission F-10 was good only in some intervals, while relationship of both Rz and F-10 with the coronal mass ejections (CMEs) was very poor, indicating that CMEs evolve independently of Rz and F-10. | en_US |
| dc.language.iso | en_US | en_US |
| dc.publisher | NISCAIR-CSIR, India | en_US |
| dc.relation.ispartof | 96.60.ph; 96.60.qd; 96.60.Tf | en_US |
| dc.rights |  CC Attribution-Noncommercial-No Derivative Works 2.5 India | en_US |
| dc.source | IJRSP Vol.40(3) [June 2011] | en_US |
| dc.subject | Coronal mass ejection (CME) | en_US |
| dc.subject | Sunspot number | en_US |
| dc.subject | Solar radio emission flux | en_US |
| dc.title | Bartel diagrams for CME occurrence frequency, sunspot numbers and 2800 MHz solar radio emission flux during 2007 | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | IJRSP Vol.40(3) [June 2011] | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| IJRSP 40(3) 121-123.pdf | 310.02 kB | Adobe PDF | View/Open |
Items in NOPR are protected by copyright, with all rights reserved, unless otherwise indicated.