Milagro (experiment)
A cosmic ray or high-energy gamma ray striking an atom in the upper atmosphere generates a cascade of particles known as an air shower. This cascade of particles are traveling near the speed of light and generate Cherenkov radiation as they pass through the atmosphere and the water in the Milagro experiment. The photons of Cherenkov radiation are detected by an array of detectors or photomultiplier tubes which send a signal to a recorder. The data from the recorder can then be used to determine the energy and direction of the cosmic or gamma ray. The Milagro experiment used 700 sensitive light detectors submerged in the pond plus another 200 detectors arrayed around the pond.
The Milagro Experiment stopped taking data in April 2008 after seven years of operation. There is a follow-up experiment called the High Altitude Water Cherenkov Experiment (HAWC) located near the Large Millimeter Telescope at the Sierra Negra volcano, Mexico, which is expected to be 15 times more sensitive. In November 2008 Milagro published the surprising result of observing cosmic ray anisotropy.
See also
Footnotes
- ^ "Los Alamos building new observatory in the Jemez". LANL Press Release. 5 May 1997. Retrieved 11 September 2010.
- ^ "Los Alamos Employee Monthly Magazine 'CURRENTS (August 08 Issue)". Retrieved 2008-12-12.
- ^ "Space Daily Two Cosmic Ray "hot spots" observed by Milagro Observatory". Retrieved 2008-12-12.
External links
- Milagro homepage at Los Alamos National Lab
- The University of Maryland HAWC page
- Los Alamos observatory fingers cosmic ray 'hot spots'
35°52′42″N 106°40′35″W / 35.87835°N 106.67625°W