'Amanda icecube' presentation slideshows

Baikal-Amanda-IceCube

Baikal-Amanda-IceCube. Neutrino-Astronmie in DESY Zeuthen. Christian Spiering, Technisches Seminar, Mai2004. Entdeckung der Kosmischen Strahlen 1912. Viktor Hess (Nobelpreis 1936). 1 TeV (HERA). Kosmische Strahlen. ?. ?. ?. Neutrino-Teleskope in Wasser und Eis. Super-K. Baikal.

760 views • 65 slides

Design and Performance of the IceCube Electronics

Design and Performance of the IceCube Electronics. R. G. Stokstad (Lawrence Berkeley National Laboratory) for the IceCube Collaboration. High Energy Neutrino Astronomy IceCube Detector DAQ and Electronics Performance Summary and Outlook. Heidelberg, September 12, 2005. ?.

634 views • 49 slides

Multi-messenger studies of point sources using AMANDA/IceCube data and strategies

420 views • 27 slides

Vrije Universiteit Brussel, Belgium

354 views • 22 slides

Julia Becker for the IceCube collaboration August 2006

Implications of neutrino flux limits. by the AMANDA experiment. Julia Becker for the IceCube collaboration August 2006. Contents. Detection principle and detector Analysis methods and results point sources stacking of point sources diffuse signal Interpretation of the diffuse signal

337 views • 19 slides

Julia Becker for the IceCube collaboration August 2006

Implications of neutrino flux limits. by the AMANDA experiment. Julia Becker for the IceCube collaboration August 2006. Contents. Detection principle and detector Analysis methods and results point sources stacking of point sources diffuse signal Interpretation of the diffuse signal

196 views • 19 slides

AJ Heroux with Teresa Montaruli

AJ Heroux with Teresa Montaruli. Playing in the Snow!!. Outline What is IceCube? History Deployment DOMS IceTop Shadow of the moon Motivation Methods Results Future Work Work done with DOMs. AMANDA was the precursor to IceCube Roughly 600 PMTs Buried at depths from 1500-2000 m

260 views • 16 slides

Neutrino Astronomy

Neutrino Astronomy. @ South Pole. AMANDA & IceCube. Why Neutrino ?. High energy photons are absorbed beyond ~ 150Mpc g HE g LE ? e - e + HE n s are unique to probe HE processes in the vicinity of cosmic accelerators HE Cosmic Rays and n s may have the same origin.

276 views • 15 slides