Ryushi Azuma

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The surfaces of solid planets are covered with a tremendous number of craters of various shape and size that reeect the geological history and rheology of the planetary surfaces. In the present study we examined crater detection and categorization system for planetary images in view of data mining from a large-scale scientiic image database. Crater(More)
T.Nonaka, T.Abu-Zayyad, M.Allen, R.Azuma, J.W.Belz, D.R.Bergman, S.A.Blake, O.Brusova, R.Cady, Z.Cao, J.Chiba, M.Chikawa , I.S.Cho, H.Fujii, T.Fujii, T.Fukuda, M.Fukushima, K.Hayashi, N.Hayashida, K.Hibino, K.Honda, P.Huentemeyer, G.Hughes,D.Ikeda, N.Inoue, D.Ivanov, S.Iwamoto, C.H.Jui, K.Kadota, F.Kakimoto, H.Kang, K.Kasahara, H.Kawai, S.Kawana, E.Kido,(More)
The air fluorescence detectors (FDs) of the Telescope Array (TA) experiment have been constructed in a dessert of Utah, USA. We can measure the longitudinal developments of EASs directly with the FDs by detecting air fluorescence lights and determine the primary energies of ultra-high energy cosmic rays. In order for accurate observation and measurements of(More)
Penumbral imaging is a technique which uses the fact that spatial information can be recovered from the shadow or penumbra that an unknown source casts through a simple large circular aperture. The size of the penumbral image on the detector can be mathematically determined as its aperture size, object size, and magnification. Conventional reconstruction(More)
  • T . Abu - Zayyad, Ryo Aida, +131 authors Z . Zundel
  • 2012
We study the anisotropy of Ultra-High Energy Cosmic Ray (UHECR) events collected by the Telescope Array (TA) detector in the first 40 months of operation. Following earlier studies, we examine event sets with energy thresholds of 10 EeV, 40 EeV, and 57 EeV. We find that the distributions of the events in right ascension and declination are compatible with(More)
The construction of the fluorescence detectors (FDs) of the Telescope Array (TA) experiment have been completed in June 2007, and the stereo observation have been started in June 2007. In this paper, we describe the development of the data acquisition (DAQ) system for the TA FD observations. The DAQ system of each TA FD station is comprised of 16 CPUs: 13(More)
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