What is the Purpose of the Cosmic Ray Observatory?

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Discussion Overview

The discussion centers around the purpose and details of a new cosmic ray observatory being constructed in Utah, known as the Telescope Array. Participants explore its operational principles, particularly in relation to Cherenkov radiation and its goal of detecting cosmic rays beyond the GKZ limit. The conversation includes references to existing observatories and relevant astrophysical concepts.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants mention that the Telescope Array operates on principles similar to other observatories, utilizing Cherenkov radiation to detect cosmic rays.
  • There is a focus on the goal of the observatory to find cosmic rays beyond the GKZ limit, with a note that a large array is necessary for this purpose.
  • One participant raises a technical question regarding the mean free path formula for cosmic rays exceeding the GKZ limit, indicating a specific interest in the interaction between cosmic rays and microwave background radiation.
  • References to related literature, such as the Stecker paper and other threads, are provided for further exploration of high-energy astrophysics.

Areas of Agreement / Disagreement

Participants express varying levels of understanding and interest in the technical aspects of cosmic rays and their detection, but no consensus is reached on specific details or implications of the observatory's findings.

Contextual Notes

The discussion includes references to specific energy thresholds (EGKZ and ECRB) and the need for further data to ascertain the existence of cosmic rays beyond the GKZ limit, highlighting the ongoing nature of research in this area.

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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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