Haruyoshi Kuno
Waseda University
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Publication
Featured researches published by Haruyoshi Kuno.
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.
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
Japan Geoscience Union | 2017
Hiroshi Nagaoka; Nobuyuki Hasebe; Masayuki Naito; Miho Mizone; Haruyoshi Kuno
The Japan Society of Applied Physics | 2016
Hiroki Kusano; Nobuyuki Hasebe; Hiroshi Nagaoka; Eido Shibamura; Yoshiharu Amano; Tohru Ohta; Timothy J. Fagan; Haruyoshi Kuno
The Japan Society of Applied Physics | 2016
Masayuki Naito; Miho Mizone; Hiroki Kusano; Eido Shibamura; Hiroshi Nagaoka; Haruyoshi Kuno; Nubuyuki Hasebe
The Japan Society of Applied Physics | 2016
Masayuki Naito; Miho Mizone; Hiroki Kusano; Hiroshi Nagaoka; Eido Shibamura; Haruyoshi Kuno; Nubuyuki Hasebe
The Japan Society of Applied Physics | 2016
Hiroki Kusano; Nobuyuki Hasebe; Hiroshi Nagaoka; Eido Shibamura; Yoshiharu Amano; Tohru Ohta; Timothy J. Fagan; Haruyoshi Kuno
Proceedings of International Symposium on Radiation Detectors and Their Uses (ISRD2016) | 2016
Hiroki Kusano; Nobuyuki Hasebe; Hiroshi Nagaoka; Masayuki Naito; Miho Mizone; Yoshiharu Amano; Eido Shibamura; Haruyoshi Kuno
Proceedings of International Symposium on Radiation Detectors and Their Uses (ISRD2016) | 2016
Hiroshi Nagaoka; Nobuyuki Hasebe; Hiroki Kusano; Yoshiharu Amano; Eido Shibamura; Tohru Ohta; Timothy J. Fagan; Masayuki Naito; Haruyoshi Kuno; José A. Matias Lopes