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Talk55 min

Recent Results from AMANDA

C Wiebusch · CERN

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About

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 detect Cherenkov light emitted by charged secondary particles, which are produced in neutrino interactions inside or close to the detector..

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The talk

  1. Recent Results from AMANDA 2001-10-01 · 55 min · CERN's player

Credits and licence

Institution
CERN
Department
CERN EP Monday Seminars,2001
Speaker
C Wiebusch
Year
2001
Language
English
Subjects
Astronomy and space
Source
CERN
Licence
CERN, as CERN states it. CERN's terms
Attribution
© CERN. CERN provides its audiovisual media free of charge for educational and informational use, credited to CERN; this lecture is shown in CERN's own player.
Who can watch
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