UHECR Study on Satellites in TUS/KLYPVE Experiments

Details UHECR Study on Satellites in TUS/KLYPVE Experiments UHECR Study on Satellites in TUS/KLYPVE Experiments

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....1..497a&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

The TUS/KLYPVE space experiments have been proposed to study the energy spectrum, composition and arrival direction of the Ultra High Energy Cosmic Rays (UHECR) by detection from the space satellites of the atmosphere fluorescence and Cherenkov light produced by UHECR initiated Extensive Atmosphere Showers (EAS). The TUS set up is a prototype of the KLYPVE. The aim of the TUS experiment is to detect a dozen of UHECR events in the energy region of the GZK cutoff, to measure the light background, to test the atmosphere control methods, to study a stability of the optic materials, of PMTs, and of DAQ in the space environment.

Affiliated with

Also associated with

No associations

Rating

UHECR Study on Satellites in TUS/KLYPVE Experiments does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with UHECR Study on Satellites in TUS/KLYPVE Experiments, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and UHECR Study on Satellites in TUS/KLYPVE Experiments will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1135985