What is the Purpose of the Cosmic Ray Observatory?

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The Cosmic Ray Observatory, specifically the Telescope Array being constructed in Utah, aims to investigate cosmic rays (CRs) beyond the Greisen-Zatsepin-Kuzmin (GKZ) limit. It utilizes Cherenkov radiation to detect these high-energy particles as they interact with the atmosphere. The observatory's extensive array is necessary for gathering sufficient data, which is expected to take four years to complete. Current research has shown limited findings on CRs exceeding the GKZ limit, highlighting the need for this new facility. This project represents a significant step in high-energy astrophysics and the understanding of cosmic ray interactions.
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Reference:
http://www.sltrib.com/2004/Jan/01132004/utah/128616.asp
 
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Astronomy news on Phys.org
this site shows a headline but no script, it may be a
temp fault, can you give any info as to what this is about?
 
A new cosmic ray observatory being built in Utah - 'the Telescope Array'. Works on the same principle as many others already built (e.g. Fly Eye), Cherenkov radiation* emitted by the charged particle rays as they encounter a medium where the speed of light is slower than the one they were in (atmosphere vs space). They're looking for CRs beyond the GKZ limit*, and to do that you need a huge array. Will take four years to build. There's been limited data to date on whether there are CRs beyond the GKZ.

For more on the whole area of high-energy astrophysics, see the Stecker paper (it's in another thread somewhere here - really interesting stuff!)

*links:
Cherenkov: http://scienceworld.wolfram.com/physics/CherenkovRadiation.html
GKZ limit: http://www.phys.washington.edu/~walta/importance.html
 
GKZ Probability...



What is the cosmic ray-microwave background radiation interaction Mean Free Path formula for cosmic rays exceeding GKZ limit?

EGKZ = 10^19 eV
ECRB >= 10^21 eV

Reference:
http://www.phys.washington.edu/~walta/importance.html

 
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