Cargando…
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...
Autor principal: | |
---|---|
Lenguaje: | eng |
Publicado: |
2006
|
Materias: | |
Acceso en línea: | http://cds.cern.ch/record/1563532 |
_version_ | 1780930768508289024 |
---|---|
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 |
record_format | invenio |
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 |