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L'effet de la temperature atmospherique sur la variation diurne des muons a haute energie du rayonnement cosmique est determine sur la base des donnees du telescope multi-directionnel a muons situe a l'observatoire souterrain de Matsushiro et compare aux autres resultats de telescopes a la surface et souterrains. La methode utilisee dans l'analyse est basee sur l'idee que la variation observee peut etre separee en 2 parties de l'origine atmospherique et extra-atmospherique en utilisant des telescopes croises

The atmospheric temperature effect on the diurnal variation of cosmic-ray muon intensity observed at 220m.w.e. underground at Matsushiro.