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               Phantom 
                    Detectors
              
             
            
            
           
            
             
               
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               Photo:
               
                John 
                        Jacobsen
               
              
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                Hoses 
                        carrying hot water melt their way into the ice. The hot 
                        water is used to drill the deep columns into which the 
                        optical sensors are placed.
               
              
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             Neutrino 
					detection is tricky business. The instrument must be big enough 
					to detect the rare neutrino interaction, transparent enough 
					to track a muon's path across a great distance, and far enough 
					below the Earth's surface to filter out interference from 
					irrelevant particles and light. As it turns out, the extraordinary 
					clarity of the deep Antarctic ice provides an ideal medium.
            
            
           
            
             Buried nearly a mile and a half beneath the Polar ice cap, 
					AMANDA acts more like a telescope than a traditional particle 
					detector, collecting rather than creating particle debris. 
					But while most telescopes search the skies with optical lenses 
					and mirrors to capture celestial light, this one uses phototubes 
					in glass orbs to scrutinize the subterranean ice for the light 
					that heralds a neutrino's passing. Nearly seven hundred of 
					these glass detectors are placed throughout the ice, strung 
					on nineteen cables lowered deep into narrow columns of melted 
					ice, where they freeze in place. You can see how these parts 
					of the detector are set up in
             
              a 
					variety of schematic diagrams of the detector
             
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             As neutrinos bombard the sunken detectors, a few interact 
                    with subatomic particles in the ice and rock and create muons. 
                    Essentially a heavy electron, the negatively charged muon 
                    emits a faint blue light that illuminates the phototubes.
            
            
           
            
             Acting like light bulbs in reverse, the phototubes collect 
                    a muon's light and convert it into electrical signals, which 
                    are sent to computers above the ice that store and process 
                    the data. The signals announce the presence of a neutrino 
                    arrival, as well as its rate, frequency, and path. Researchers 
                    hope to trace the muon's path back to the neutrino's cosmic 
                    origins.
            
            
           
            
             To mine the full potential of the deep, clear Antarctic ice, 
					scientists plan to outfit AMANDA with as many as 50,000 orbs 
					on 80 cables over the next decade. As they push the limits 
					of engineering and endurance, researchers sense the discovery 
					of something truly monumentalthough they're not sure 
					what. They'll just have to wait till the heavens send them 
					the clues.
            
            
           
            
             
              
               To learn more about AMANDA:
              
             
            
            
           
            
             AMANDA Web page:
              
             
              http://amanda.berkeley.edu/amanda/amanda.html
             
            
            
           
            
             The Center for Astrophysical Research in Antarctica:
              
             
              http://astro.uchicago.edu/cara/home.html
             
            
            
           
             
            
           
           
             
            
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