Please use this identifier to cite or link to this item:
http://nopr.niscpr.res.in/handle/123456789/36003Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Bala, B | - |
| dc.contributor.author | Nayar, S R Prabhakaran | - |
| dc.date.accessioned | 2016-10-24T08:07:03Z | - |
| dc.date.available | 2016-10-24T08:07:03Z | - |
| dc.date.issued | 1993-08 | - |
| dc.identifier.issn | 0975-105X (Online); 0367-8393 (Print) | - |
| dc.identifier.uri | http://nopr.niscair.res.in/handle/123456789/36003 | - |
| dc.description | 273-276 | en_US |
| dc.description.abstract | Azimuthal variation of solar wind velocity in the range 300-450 km s-1 has been found to exist along the current sheet during 1972-1977. The possibility of using the Ap index (when the earth goes through an IMF sector boundary crossing) to study the azimuthal structure of solar wind has been analysed. The longitudinal variation of the Ap index in terms of Carrington longitude is found to be similar to that of the solar wind velocity variation. | 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.22(4) [August 1993] | en_US |
| dc.title | Structure of solar wind velocity along the HCS and related geomagnetic field variations | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | IJRSP Vol.22(4) [August 1993] | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| IJRSP 22(4) 273-276.pdf | 353.79 kB | Adobe PDF | View/Open |
Items in NOPR are protected by copyright, with all rights reserved, unless otherwise indicated.