Status report on the EUSO project at the end of phase A

Abstract : EUSO is 2.5 m diameter telescope to be installed on the International Space Station (ISS) to observe from above ($\sim$400 km altitude), very high energy ($10^10-21$eV) cosmic rays by detecting the UV light generated by the billions of electrons in the shower ionizing the atmosphere nitrogen. The European and Japanese parts of the collaboration depend on ESA for the mission and the results of phase A should be examined in November 2003.The US part of the collaboration has already been approved for phase B by NASA, to the condition of an OK by ESA.
Type de document :
Communication dans un congrès
Frank Avignone, Wick Haxton. International Workshop on Topics in Astroparticle and Undeground, TAUP 2003, Sep 2003, Seattle, United States. 138, pp.183-186, 2005, <10.1016/j.nuclphysbps.2004.11.043>


http://hal.in2p3.fr/in2p3-00024527
Contributeur : Simone Lantz <>
Soumis le : lundi 5 septembre 2005 - 16:39:31
Dernière modification le : mercredi 12 octobre 2016 - 01:16:52

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PCC | PSL | USPC

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P. Gorodetzky. Status report on the EUSO project at the end of phase A. Frank Avignone, Wick Haxton. International Workshop on Topics in Astroparticle and Undeground, TAUP 2003, Sep 2003, Seattle, United States. 138, pp.183-186, 2005, <10.1016/j.nuclphysbps.2004.11.043>. <in2p3-00024527>

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