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Recent Results from AMANDA
The main aim of the AMANDA-Experiment at the South Pole is the detection of High Energy (> TeV) Neutrinos of galactic or extra-galactic origin. For this reason large photomultipliers, mounted in pressure spheres, are deployed into the deep (> 1.5km) Antarctic glacier. These photomultipliers de...
Autor principal: | Wiebusch, C |
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Lenguaje: | eng |
Publicado: |
2001
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Materias: | |
Acceso en línea: | http://cds.cern.ch/record/529961 |
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