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| Image #PN004 |
Belle CsI |
Dec. 1998 |
Csl calorimeter is being assembled into the Belle detector in the Tsukuba Experimental Hall
by Tokio Ohska |
| mid-res image : hi-res image |
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| Image #PN005 |
Belle Event |
Nov 2,2001 |
Example of a fully reconstructd evrnt in the Belle detector.
by Belle Collaboration |
| mid-res image : hi-res image |
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| Image #PN007 |
T2K Neutrino Beam Line |
Jul 17, 2008 |
| T2K (Tokai to Kamioka) neutrino beam line nears completion. Built inside the 50 GeV synchrotron, 28 multifunctional quad-dipole superconducting magnets will bend proton beams toward toward Super-Kamiokande, 300 km away neutrino detector.
by A. Yamanaka |
| mid-res image : hi-res image |
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| Image #PN008 |
T2K Neutrino Beam Line |
Jul 17, 2008 |
T2K (Tokai to Kamioka) neutrino beam line nears completion. Built inside the 50 GeV synchrotron, 28 multifunctional quad-dipole superconducting magnets will bend proton beams toward toward Super-Kamiokande, 300 km away neutrino detector.
by A. Yamanaka |
| mid-res image : hi-res image |
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| Image #PN010 |
K2K Near Detector |
Feb, 1999 |
Consisting of a 1kton water Cerenkov detector and a fine-grained detector for Long-baseline Neutrino Oscillation Experiment. The near detector system is located at 300m downstream of the KEK PS beamline production target.
by Tokio Ohska |
| mid-res image : hi-res image |
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| Image #PN011 |
K2K Neutrino Beam line |
May 6, 1999 |
Electric Magnet Horn in the Neutrino Beam Line for the K2K experiment.
by Tokio Ohska |
| mid-res image : hi-res image |
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| Image #PN012 |
K2K Neutrino Beam line |
May 6, 1999 |
Beam line for K2K neutrino experiment.
by Tokio Ohska |
| mid-res image : hi-res image |
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| Image #PN013 |
K2K neutrino events |
Fev 26,2000 |
Neutrino event detected by the Super-KAMIOKANDE of the K2K experiment.
by K2K Collaboration |
| mid-res image : hi-res image |
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| Image #PN014 |
K2K neutrino events |
mar 6 1999 |
Neutrino event detected by the near detector of the K2K experiment.
by K2K Collaboration |
| mid-res image : hi-res image |
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| Image #PN015 |
K2K neutrino events |
Jun 19,1999 |
The First K2K event at Super-KAMIOKANDE
by K2K Collaboration |
| mid-res image : hi-res image |
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| Image #PN016 |
BESS |
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BESS collaboration launches a 130 m wide balloon in Alberta, Canada. Once launched, a 2.3 ton detector is airborne for about 24 hours at an altitude of 37 km in the stratosphere, in search of anti-nucleus in the cosmic ray. If any abundances of anti-helium flux were to be found in the data, it might indicate the existence of "anti-matter galaxy". Researchers from KEK has built a compact and light weight superconducting solenoid for the detector.
by BESS Collaboration |
| mid-res image : hi-res image |
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| Image #PN017 |
BESS |
Dec 13, 2004 |
BESS-Polar instrument, launched successfully on December 13 from McMurdo Station, Antarctica, beneath a 40-million-cubic-foot scientific balloon, as big as a football field. To maximize the possibility of finding the antimatter predicted by Hawking, the team is hoping for at least a 10-day flight, or once around the South Pole, in a near-space environment above 99% of the atmosphere. The instrument is circling the Pole at an average altitude of 24 miles (39 kilometers).
BESS-Polar is collaboration among scientists at KEK, the University of Tokyo, Kobe University, and the Institute of Space and Astronautical Science of the Japan Aerospace Exploration Agency, along with NASA and the University of Maryland, College Park. BESS stands for Balloon-borne Experiment with a Superconducting Spectrometer.
by BESS Collaboration |
| mid-res image : hi-res image |
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| Image #PN018 |
BESS |
Dec 13, 2004 |
BESS-Polar instrument, launched successfully on December 13 from McMurdo Station, Antarctica, beneath a 40-million-cubic-foot scientific balloon, as big as a football field. To maximize the possibility of finding the antimatter predicted by Hawking, the team is hoping for at least a 10-day flight, or once around the South Pole, in a near-space environment above 99% of the atmosphere. The instrument is circling the Pole at an average altitude of 24 miles (39 kilometers).
BESS-Polar is collaboration among scientists at KEK, the University of Tokyo, Kobe University, and the Institute of Space and Astronautical Science of the Japan Aerospace Exploration Agency, along with NASA and the University of Maryland, College Park. BESS stands for Balloon-borne Experiment with a Superconducting Spectrometer.
by BESS Collaboration |
| mid-res image : hi-res image |
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| Image #PN019 |
BESS |
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BESS event observed in the 1999 Alberta-Canada campaign.
A 1.18 GeV positive particle penetrated the
tracking chamber from top to bottom.
by BESS Collaboration |
| mid-res image : hi-res image |
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