Masayuki Naito
Waseda University
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Featured researches published by Masayuki Naito.
Proceedings of SPIE | 2014
Hiroki Kusano; Yuki Oyama; Masayuki Naito; Hiroshi Nagaoka; Haruyoshi Kuno; Eido Shibamura; Nobuyuki Hasebe; Yoshiharu Amano; Kyeong Ja Kim; José A. Matias Lopes
The chemical element abundance on planetary surface is essential for planetary science. We have been developing an active X-ray spectrometer (AXS), which is an in-situ chemical element analyzer based on the X-ray florescence analysis for future planetary landing missions. The AXS consists of an X-ray detector and multiple X-ray sources. Although a pyroelectric X-ray generator is promising for the AXS as an X-ray source, the raise of emission X-ray intensity is necessary for short-time and precise determination of elemental composition. Also, in order to enhance the detection efficiency of light major elements such as Mg, Al, and Si, we have tested the low energy X-ray emission by changing the target material. In this study, the X-ray emission calculation at the target by Monte Carlo simulation and the X-ray emission experiments were carried out. More than 106 cps of the time-averaged X-ray emission rate was achieved in maximum using a LiTaO3 crystal with 4 mm thickness and Cu target with 10 um thickness. The performance of pyroelectric X-ray generator is presented in this paper.
Hard X-Ray, Gamma-Ray, and Neutron Detector Physics XIX 2017 | 2017
Masayuki Naito; Nobuyuki Hasebe; Hiroshi Nagaoka; Yusuke Oshima; Miho Mizone; Eido Shibamura; Haruyoshi Kuno; Kyeong Ja Kim; José A. Matias-Lopes; Jesús Martínez-Frías
The elemental composition on planetary surface provides us an essential information to improve geological and geochemical understanding of planets. An active X-ray spectrometer (AXS) was developed and proposed as one of the mission payloads to perform in-situ X-ray fluorescence analysis. The AXS consists of multiple pyroelectric X-ray generators (PXGs) and a silicon drift detector (SDD). Although the PXG is light in weight and low in electric consumption, the limited X-ray intensity and reproducibility hamper obtaining the elemental composition by short time observation. This is attributed mainly to the less known mechanism of X-ray and electron emission by the pyroelectric crystal. In this study, we observed the crystal surface during X-ray emission as a function of the distance between the crystal top and a Cu target. Two types of light emission derived from the electric discharge were observed. The dependence of light emission on the distance was found to be related with the physical mechanism of pyroelectric X-ray emission. The study provides clues to obtain high intensity and reproducible X-rays emission. The experimental results and discussion are presented in this paper.
Hard X-Ray, Gamma-Ray, and Neutron Detector Physics XIX 2017 | 2017
Masayuki Naito; Nobuyuki Hasebe; Hiroshi Nagaoka; Junya Ishii; Daisuke Aoki; Eido Shibamura; Kyeong Ja Kim; José A. Matias-Lopes; Jesús Martínez-Frías
The elemental composition and its distribution on planetary surface provide important constraints on the origin and evolution of the planetary body. The nuclear spectrometer consisting of a neutron spectrometer and a gamma-ray spectrometer obtains elemental compositions by remote sensing. Especially, the neutron spectrometer is able to determine the hydrogen concentration, a piece of information that plays an important role in thermal history of the planets. In this work, numerical and experimental studies on the neutron spectrometer for micro-satellite application were conducted. It is found that background count rate of neutron produced from micro-satellite is very small, which enables to obtain successful results in short time observation. The neutron spectrometer combining a lithium-6 glass scintillator with a boron loaded plastic scintillator was used to be able to detect neutrons in different energy ranges. It was experimentally confirmed that the neutron signals from these scintillators were successfully discriminated by the difference of scintillation decay time between two detectors. The measurement of neutron count rates of two scintillators is found to determine hydrogen concentration on the planetary surfaces in the future missions.
conference of the industrial electronics society | 2014
Sota Shimizu; Takumi Kadogawa; Masayuki Naito; Takumi Hashizume; Hiroki Kusano; Hiroshi Nagaoka; Nobuyuki; Hasebe; Yoshiaki Tanzawa
There exists a well-known visual illusion with respect to color propagation. That is, a human subject confuses a color in the subjects peripheral field of view (FOV) as another color in the central FOV (with a shape of circular disk) spreads into the peripheral FOV or as a color in the peripheral FOV erodes another color in the central FOV (also with a shape of circular disk) when he/she keeps gazing at a specific color visual stimulus in his/her central FOV for more than several seconds. In this paper, the authors experiment this illusion using multiple naive subjects in conditions of the visual stimuli as the central or peripheral colors and the disk size change. This paper has proposed a rate of propagation as a criterion and has analyzed and discussed the illusion using it.
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2015
Masayuki Naito; N. Hasebe; Hiroki Kusano; Hiroshi Nagaoka; M. Kuwako; Yuki Oyama; Eido Shibamura; Yoshiharu Amano; Tohru Ohta; Kyeong Ja Kim; J. A. M. Lopes
Proceedings of International Symposium on Radiation Detectors and Their Uses (ISRD2016) | 2016
Masayuki Naito; Nobuyuki Hasebe; Kouhei Yoshida; Junya Ishii; Daisuke Aoki; Hiroshi Nagaoka; Hiroki Kusano; Eido Shibamura
Transactions of The Japan Society for Aeronautical and Space Sciences, Space Technology Japan | 2018
Hiroshi Nagaoka; Nobuyuki Hasebe; Masayuki Naito; Eido Shibamura; Haruyoshi Kuno; Miho Mizone; Kyeong Ja Kim
Journal of Geoscience and Environment Protection | 2018
Masayuki Naito; Nobuyuki Hasebe; Junya Ishii; José A. Matias-Lopes; V. V. Dmitrenko; Christian Wöhler; Kyeong Ja Kim
The Japan Society of Applied Physics | 2017
Junya Ishii; Nobuyuki Hasebe; Hiroshi Nagaoka; Masayuki Naito; Aoki Daisuke; Kimura Yuri
Japan Geoscience Union | 2017
Hiroshi Nagaoka; Nobuyuki Hasebe; Masayuki Naito; Miho Mizone; Haruyoshi Kuno