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Exploring the cosmic rays energy frontier with the Auger Observatory

<!--HTML-->The existence of cosmic rays with energies in excess of 10<sup>20</sup> eV represents a longstanding scientific mystery. Unveileing the mechanism and source of production/acceleration of particles of such enormous energies is a challenging experimental task due to their...

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Autor principal: PRIVITERA (University Roma II)
Lenguaje:eng
Publicado: 2006
Materias:
Acceso en línea:http://cds.cern.ch/record/1563532
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author PRIVITERA (University Roma II)
author_facet PRIVITERA (University Roma II)
author_sort PRIVITERA (University Roma II)
collection CERN
description <!--HTML-->The existence of cosmic rays with energies in excess of 10<sup>20</sup> eV represents a longstanding scientific mystery. Unveileing the mechanism and source of production/acceleration of particles of such enormous energies is a challenging experimental task due to their minute flux, roughly one km<sup>2</sup> century.<br /><br> The Pierre Auger Observatory, now nearing completion in Malargue, Mendoza Province, Argentina, is spread over an area of 3000 km<sup>2</sup>. Two techniques are employed to observe the cosmic ray showers: detection of the shower particles on the ground and detection of fluorescence light produced as the shower particles pass through the atmosphere. I will describe the status of the Observatory and its detectors, and early results from the data recorded while the observatory is reaching its completion.<BR><BR><I>Organiser(s): L. Alvarez-Gaume / PH-TH</I><BR><BR><I>Note: * Tea & coffee will be served at 16:00.</I>
id cern-1563532
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2006
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spelling cern-15635322022-11-02T22:19:48Zhttp://cds.cern.ch/record/1563532engPRIVITERA (University Roma II)Exploring the cosmic rays energy frontier with the Auger ObservatoryExploring the cosmic rays energy frontier with the Auger ObservatoryCERN Colloquium<!--HTML-->The existence of cosmic rays with energies in excess of 10<sup>20</sup> eV represents a longstanding scientific mystery. Unveileing the mechanism and source of production/acceleration of particles of such enormous energies is a challenging experimental task due to their minute flux, roughly one km<sup>2</sup> century.<br /><br> The Pierre Auger Observatory, now nearing completion in Malargue, Mendoza Province, Argentina, is spread over an area of 3000 km<sup>2</sup>. Two techniques are employed to observe the cosmic ray showers: detection of the shower particles on the ground and detection of fluorescence light produced as the shower particles pass through the atmosphere. I will describe the status of the Observatory and its detectors, and early results from the data recorded while the observatory is reaching its completion.<BR><BR><I>Organiser(s): L. Alvarez-Gaume / PH-TH</I><BR><BR><I>Note: * Tea & coffee will be served at 16:00.</I>oai:cds.cern.ch:15635322006
spellingShingle CERN Colloquium
PRIVITERA (University Roma II)
Exploring the cosmic rays energy frontier with the Auger Observatory
title Exploring the cosmic rays energy frontier with the Auger Observatory
title_full Exploring the cosmic rays energy frontier with the Auger Observatory
title_fullStr Exploring the cosmic rays energy frontier with the Auger Observatory
title_full_unstemmed Exploring the cosmic rays energy frontier with the Auger Observatory
title_short Exploring the cosmic rays energy frontier with the Auger Observatory
title_sort exploring the cosmic rays energy frontier with the auger observatory
topic CERN Colloquium
url http://cds.cern.ch/record/1563532
work_keys_str_mv AT priviterauniversityromaii exploringthecosmicraysenergyfrontierwiththeaugerobservatory