In:
International Journal of Modern Physics A, World Scientific Pub Co Pte Ltd, Vol. 16, No. supp01c ( 2001-09), p. 1013-1015
Abstract:
We present results based on data taken in 1997 with the 302-PMT Antarctic Muon and Neutrino Detector Array-B10 ("AMANDA-B10") array. Atmospheric neutrinos created in the northern hemisphere are observed indirectly through their charged current interactions which produce relativistic, Cherenkov-light-emitting upgoing muons in the South Pole ice cap. The reconstructed angular distribution of these events is in good agreement with expectation and demonstrates the viability of this ice-based device as a neutrino telescope.
Type of Medium:
Online Resource
ISSN:
0217-751X
,
1793-656X
DOI:
10.1142/S0217751X01008746
Language:
English
Publisher:
World Scientific Pub Co Pte Ltd
Publication Date:
2001
SSG:
16,12
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