Please use this identifier to cite or link to this item: http://nopr.niscair.res.in/handle/123456789/10926
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dc.contributor.authorSingh, Kamlesh-
dc.contributor.authorShrivastava, Pankaj K-
dc.date.accessioned2011-01-13T09:46:23Z-
dc.date.available2011-01-13T09:46:23Z-
dc.date.issued2010-12-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://hdl.handle.net/123456789/10926-
dc.description341-345en_US
dc.description.abstractAn extensive study of tri-diurnal anisotropy of cosmic ray daily variations for the period 1996 – 2006 has been carried out using cosmic ray neutron monitor data of Kiel and Beijing. The daily and yearly averages of tri-diurnal wave amplitude and phase have been obtained to observe long term behaviour of third harmonic of cosmic ray daily variation. The relation between amplitudes and phases (annual and daily averages) of tri-diurnal data for these two different cut off rigidities has been shown. No long-term variational trend is seen in tri-diurnal anisotropy. On day-to-day analysis, a well defined peak in tri-diurnal amplitude between 0.06% and 0.010% is observed.en_US
dc.language.isoen_USen_US
dc.publisherNISCAIR-CSIR, Indiaen_US
dc.relation.ispartof96.50.sben_US
dc.rights CC Attribution-Noncommercial-No Derivative Works 2.5 Indiaen_US
dc.sourceIJRSP Vol.39(6) [December 2010]en_US
dc.subjectCosmic raysen_US
dc.subjectTri-diurnal anisotropyen_US
dc.subjectSolar activityen_US
dc.titleTri-diurnal anisotropy of cosmic ray daily variation for the solar cycle 23en_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.39(6) [December 2010]

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