Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5602
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dc.contributor.authorMohanty, P.K.en_US
dc.contributor.authorSUBRAMANIAN, PRASAD et al.en_US
dc.coverage.spatialBexco, Busan, Koreaen_US
dc.date.accessioned2021-02-05T06:14:06Z-
dc.date.available2021-02-05T06:14:06Z-
dc.date.issued2018-08en_US
dc.identifier.citationVolume 301- 35th International Cosmic Ray Conference (ICRC2017) - Session Solar & Heliospheric. SH-Transient solar phenomena (SEP, GLE, Forbush decreases)en_US
dc.identifier.isbn-en_US
dc.identifier.issn-en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5602-
dc.identifier.urihttps://pos.sissa.it/301/357/en_US
dc.description.abstractThe GRAPES-3 experiment in Ooty, India has been operating a large area (560m22) tracking muon telescope since 2000. It consists of 16 identical modules and each one is designed to measure the flux of muons in 13 ×× 13 directions covering 2.3 sr field of view. The high statistics data has enabled to probe transient space weather events on time scale of minutes. Due to independent nature of operation of the modules, despite intermittent failure of individual modules, a continuity in rate could still be achieved. By correcting for transient instrumental problems and gradual efficiency variations, an uninterrupted muon record is being assembled which may prove to be a valuable database for probing both transient and long-term solar phenomena. Details of the efficiency correction technique will be presented during the conference.en_US
dc.language.isoenen_US
dc.publisherSissa Medialab srlen_US
dc.subjectGRAPES-3en_US
dc.subjectPhysicsen_US
dc.subject2018en_US
dc.titleLong-term correction of GRAPES-3 muon telescope efficiencyen_US
dc.typeConference Papersen_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.doihttps://doi.org/10.22323/1.301.0357en_US
dc.identifier.sourcetitleVolume 301- 35th International Cosmic Ray Conference (ICRC2017) - Session Solar & Heliospheric. SH-Transient solar phenomena (SEP, GLE, Forbush decreases)en_US
dc.publication.originofpublisherForeignen_US
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