Conveners
Astroparticle Detectors
- Hiroyasu TAJIMA (SLAC)
Astroparticle Detectors
- Ronaldo Bellazzini (INFN Pisa)
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Oliver Grimm (ETH Zurich)12/02/2013, 14:00TalkSolar Orbiter is a sun-observing mission of the European Space Agency, addressing the interaction between the sun and the heliosphere (launch is scheduled for 2017). The satellite will carry ten instruments, and will approach the sun to 0.28 astronomical units, allowing unprecedented high-resolution measurements. The X-ray imaging spectrometer on-board Solar Orbiter is called STIX...Go to contribution page
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Dr Nicola Mori (INFN Florence)12/02/2013, 14:25TalkCalorimetry plays an essential role in experiments for observing very high energy gamma and cosmic rays in space. Geometrical dimensions and mass of the calorimeter are the main limiting factors. The available mass depends on the design of the detector and the total available mass of the payload. It is therefore important to optimize the geometrical acceptance of the calorimeter for rare...Go to contribution page
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Dr Giuseppe Osteria (INFN Napoli)12/02/2013, 14:50TalkThe JEM-EUSO instrument is a wide-angle refractive telescope in near-UV wavelength region being proposed for attachment to the Japanese Experiment Module onboard ISS. The main scientific goal of the mission is the study of Ultra High Energy cosmic Rays. The instrument consists of high transmittance optical Fresnel lenses with a diameter of 2.5 m, a focal surface covered by 4932 MAPMTs of 64...Go to contribution page
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Nikolay Budnev (Irkutsk State University)12/02/2013, 15:15TalkIn autumn of 2012 a EAS Cherenkov light array Tunka-133 with $\sim$3\,km$^2$ geometrical area in the Tunka Valley (50 km from Lake Baikal) for a detailed study of the cosmic ray energy spectrum and the mass composition with energy above 10$^{16}$ eV was combined with new Tunka-Rex (Tunka radio extension) array of about 20 antennas measures the radio emission of cosmic-ray air showers. The...Go to contribution page
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Dr Zhiguo Yao (IHEP, Beijing)12/02/2013, 16:30TalkLarge Area Water Cherenkov Array (LAWCA), a newly planned water Cherenkov detector, is to be built in Yangbajing, Tibet, China by the end of 2014, for detecting air showers at high altitude of 4300 m a.s.l. The LAWCA detector, amounting to an area of 23,000 m2 and built adjacent to the ARGO-YBJ detector, mainly aims to all sky survey for transient sources. A cross calibration between LAWCA and...Go to contribution page
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takaaki mori12/02/2013, 16:55TalkIn the universe, there exist supernova relic neutrinos (SRN) which have been released from all past supernova explosions. Super Kamiokande (SK) has conducted search for these SRN events via inverse beta decay interaction in the detector, and it is about to reach the SRN signals with sensitivity of about a factor of 2. But, it is still difficult to observe them since the search is limited by...Go to contribution page
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Seiko Hirota (Kyoto University)12/02/2013, 17:20TalkA hybrid photo-detector (HPD) is being developed for the Hyper-Kamiokande experiment, a next-generation underground water Cherenkov detector designed to study a wide range of topics in physics and astronomy. To establish the feasibility of HPDs for Hyper-Kamiokande, we plan to study their long-term stability and determine their neutrino detection performance. The HPD is a hybridization of a...Go to contribution page