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Neutrino IceCube

The contemporary observation of the full sky with at least two neutrino telescopes in opposite Earth Hemispheres is an important issue for the study of transient phenomena. Moreover v events detection from the Northern Hemisphere is required to observe the Galactic Centre region (not seen by ICECUBE), already observed by HESS as an intense TeV gamma source. In the Norther Hemisphere a favourable region is offered by the Mediterranean Sea, where several abyssal sites (> 3000 m) close to the coast are present and where it is possible to install the detector near scientific and industrial infrastructures. [Pg.232]

In the South Pole the ICECUBE detector is extending AMANDA to the km3 size and it is planned to be completed within year 2010, being probably the fist km3 telescope running. In the Mediterranean Sea ANTARES is going to install a 0.1 km2 neutrino telescope demonstrator, NESTOR has deployed... [Pg.238]

See other pages where Neutrino IceCube is mentioned: [Pg.274]    [Pg.311]    [Pg.312]    [Pg.219]    [Pg.231]    [Pg.231]    [Pg.232]    [Pg.276]   
See also in sourсe #XX -- [ Pg.232 ]



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