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http://nopr.niscpr.res.in/handle/123456789/37977Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Srivastava, B. J. | - |
| dc.contributor.author | Abbas, Habiba | - |
| dc.date.accessioned | 2016-12-01T07:06:22Z | - |
| dc.date.available | 2016-12-01T07:06:22Z | - |
| dc.date.issued | 1973-09 | - |
| dc.identifier.issn | 0975-105X (Online); 0367-8393 (Print) | - |
| dc.identifier.uri | http://nopr.niscair.res.in/handle/123456789/37977 | - |
| dc.description | 177-179 | en_US |
| dc.description.abstract | The rise-times of SSCs are found to range from 1 to 8 min and the amplitudes from 5 to 100 γ. An inverse relationship (negative correlation) has been obtained between the rise-time and the amplitude of SSCS at Hyderabad, similar to Alibag and Hermanus, but quite different from that observed for Budkov where a direct relationship (positive correlation) has been reported. SSC* events which are very rare at Hyderabad, are observed only during daytime and correspond to prominent events in the equatorial electrojet region. At high-latitude stations like Hartland, Eskdalemuir and Lerwick, SSC*s are observed both during day and night hours. The implications of these observations are examined. The observed association of micro-pulsations with SSCs and SSC*s is also discussed. | 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.02(3) [September 1973] | en_US |
| dc.title | Some Aspects of SSCs Observed at Hyderabad during 1965-72 | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | IJRSP Vol.02(3) [September 1973] | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| IJRSP 2(3) 177-179.pdf | 292.67 kB | Adobe PDF | View/Open |
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