Results from the Pierre Auger Observatory

dc.contributor.authorŠmída, R.
dc.date.accessioned2017-06-04T18:39:33Z
dc.date.available2017-06-04T18:39:33Z
dc.date.issued2012
dc.description.abstractThe Pierre Auger Observatory is the largest observatory of high-energy cosmic rays. It is located in Argentina and has been taking data since January 2004. Extensive air showers initiated by cosmic rays are measured by the hybrid detector, which combines the sampling of particle density at ground by water-Cherenkov tanks and the measurement of atmospheric fluorescence light by telescopes. New detection techniques, like radio and microwave measurement, are also being tested. Results regarding the energy spectrum, mass composition and arrival directions of cosmic rays are presented here.uk_UA
dc.identifier.citationResults from the Pierre Auger Observatory / R. Šmída // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 1. — С. 67-72. — Бібліогр.: 22 назв. — англ.uk_UA
dc.identifier.issn2227-1481
dc.identifier.urihttps://nasplib.isofts.kiev.ua/handle/123456789/119176
dc.language.isoenuk_UA
dc.publisherГоловна астрономічна обсерваторія НАН Україниuk_UA
dc.relation.ispartofAdvances in Astronomy and Space Physics
dc.statuspublished earlieruk_UA
dc.titleResults from the Pierre Auger Observatoryuk_UA
dc.typeArticleuk_UA

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