Please use this identifier to cite or link to this item: http://nopr.niscair.res.in/handle/123456789/37315
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dc.contributor.authorNigam, S K-
dc.contributor.authorSingh, R L-
dc.contributor.authorAgrawal, S P-
dc.date.accessioned2016-11-23T06:08:18Z-
dc.date.available2016-11-23T06:08:18Z-
dc.date.issued1978-08-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://nopr.niscair.res.in/handle/123456789/37315-
dc.description200-204en_US
dc.description.abstractThe influence of interplanetary magnetic field sector structure and its boundary crossing on daily variation of cosmic ray intensity has been investigated for the years 1970-76, a period of declining solar activity and occurrence of unusually large high velocity solar wind streams. Its relationship with other correlated variables such as solar wind velocity (V),å Kp and mean intensity of the cosmic rays (I), shows a consistent behaviour throughout the period. It is found that, in general, the amplitude of the diurnal variation on the day of sector boundary crossing is lowest, wherea3 the time of maximum seems to be unperturbed. These results along with its effect on V, å Kp and I are reported and discussed.en_US
dc.language.isoen_USen_US
dc.publisherNISCAIR-CSIR, Indiaen_US
dc.rights CC Attribution-Noncommercial-No Derivative Works 2.5 Indiaen_US
dc.sourceIJRSP Vol.07(4) [August 1978]en_US
dc.titleInterplanetary Magnetic Field Sector Structure & Its Effect on Cosmic Ray Diurnal Variationen_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.07(4) [August 1978]

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