Neutrino detection in AMANDA detector

Neutrino detection in AMANDA detector

A142/0470 Rights Managed

Request low-res file

530 pixels on longest edge, unwatermarked

Request/Download high-res file

Uncompressed file size: 24.2MB

Downloadable file size: 479.3KB

Price image Pricing

Please login to use the price calculator


Caption: Cosmic neutrino. The computer reconstruction shows the path of a muon (blue line), created by a cosmic neutrino, in the AMANDA detector at the South Pole. AMANDA consists of strings of phototubes (white lines) buried up to 2400 m deep in the Antarctic ice. The phototubes detect faint Cerenkov radiation emitted when high-speed muons travel through the ice. By recording the time (figures showing nanoseconds) after the first light is recorded, the muon's direction can be calculated. Its upward track indicates it was created when a neutrino that had travelled all the way through the earth from the northern hemisphere interacted in the ice or rock beneath AMANDA.

Release details: Model release not required. Property release not required.

Keywords: amanda detector, computer screen, cosmic rays, electronic display, high-energy physics, leptons, muons, neutrinos, particle physics research, south pole, subatomic particles, the particle odyssey

Licence fees: A licence fee will be charged for any media (low or high resolution) used in your project.