Digital Repository

Long-term correction of GRAPES-3 muon telescope efficiency

Show simple item record

dc.contributor.author Mohanty, P.K. en_US
dc.contributor.author SUBRAMANIAN, PRASAD et al. en_US
dc.coverage.spatial Bexco, Busan, Korea en_US
dc.date.accessioned 2021-02-05T06:14:06Z
dc.date.available 2021-02-05T06:14:06Z
dc.date.issued 2018-08 en_US
dc.identifier.citation Volume 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.uri http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5602
dc.identifier.uri https://pos.sissa.it/301/357/ en_US
dc.description.abstract The 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.iso en en_US
dc.publisher Sissa Medialab srl en_US
dc.subject GRAPES-3 en_US
dc.subject Physics en_US
dc.subject 2018 en_US
dc.title Long-term correction of GRAPES-3 muon telescope efficiency en_US
dc.type Conference Papers en_US
dc.contributor.department Dept. of Physics en_US
dc.identifier.doi https://doi.org/10.22323/1.301.0357 en_US
dc.identifier.sourcetitle Volume 301- 35th International Cosmic Ray Conference (ICRC2017) - Session Solar & Heliospheric. SH-Transient solar phenomena (SEP, GLE, Forbush decreases) en_US
dc.publication.originofpublisher Foreign en_US


Files in this item

Files Size Format View

There are no files associated with this item.

This item appears in the following Collection(s)

Show simple item record

Search Repository


Advanced Search

Browse

My Account