Results from the Pierre Auger Observatory

dc.contributor.author	Šmída, R.
dc.date.accessioned	2017-06-04T18:39:33Z
dc.date.available	2017-06-04T18:39:33Z
dc.date.issued	2012
dc.identifier.citation	Results 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.issn	2227-1481
dc.identifier.uri	http://dspace.nbuv.gov.ua/handle/123456789/119176
dc.description.abstract	The 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.language.iso	en	uk_UA
dc.publisher	Головна астрономічна обсерваторія НАН України	uk_UA
dc.relation.ispartof	Advances in Astronomy and Space Physics
dc.title	Results from the Pierre Auger Observatory	uk_UA
dc.type	Article	uk_UA
dc.status	published earlier	uk_UA