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VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
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SEQUENCE:0
UID:UW-Physics-Event-2029
DTSTART:20101208T200000Z
DURATION:PT1H0M0S
DTSTAMP:20260506T161521Z
LAST-MODIFIED:20101208T174128Z
LOCATION:4274 Chamberlin
SUMMARY:Pierre Auger Neutrino Measurement\, NPAC (Nuclear/Particle/Ast
 ro/Cosmo) Forum\, Lukas Nellen\, UNAM
DESCRIPTION:The Pierre Auger Observatory is currently the world's larg
 est cosmic ray<br>
\nobservatory. The southern site\, in Malarguee\, M
 endoza\, Argentia\, covers<br>
\n3000 km^2\, instrumented with more th
 an 1600 water Cherenkov detectors and<br>
\n24 fluorescence telescopes
 .<br>
\n<br>
\nI will present the status of the Pierre Auger Observato
 ry and its recent<br>
\nresults. Even though the obesravtory was desig
 ned primarily as a detector<br>
\nfor charged cosmic rays\, was clear 
 from the beginning that it can also<br>
\nidentify photons and neutrin
 os. I will discuss the methods for the<br>
\nidentification of the pri
 mary cosmic rays\, with emphasis on neutrino<br>
\ntagging\, and prese
 nt the flux limits obtained.
URL:https://www.physics.wisc.edu/events/?id=2029
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