Future lunar mission Active X-ray Spectrometer development: Surface roughness and geometry studies

被引:5
|
作者
Naito, M. [1 ]
Hasebe, N. [1 ,2 ]
Kusano, H. [2 ]
Nagaoka, H. [1 ,2 ]
Kuwako, M. [1 ]
Oyama, Y. [1 ]
Shibamura, E. [2 ]
Amano, Y. [2 ]
Ohta, T. [3 ]
Kim, K. J. [4 ]
Lopes, J. A. M. [5 ,6 ]
机构
[1] Waseda Univ, Sch Adv Sci & Engn, Shinjuku Ku, Tokyo, Japan
[2] Waseda Univ, Res Insulate Sci & Engn, Shinjuku Ku, Tokyo, Japan
[3] Waseda Univ, Sch Educ & Integrated Arts & Sci, Shinjuku Ku, Tokyo, Japan
[4] Korea Inst Geosci & Mineral Resources, Taejon 305350, South Korea
[5] Univ Coimbra, Dept Phys, P-3001401 Coimbra, Portugal
[6] Inst Super Engn Coimbra, P-3030199 Coimbra, Portugal
关键词
The moon; X-ray fluorescence; Active X-ray Spectrometer; REFERENCE SAMPLES; 1994; COMPILATION; PROBE;
D O I
10.1016/j.nima.2015.03.083
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
The Active X-ray Spectrometer (AXS) is considered as one of the scientific payload candidates for a future Japanese mission, SELENE-2. The AXS consists of pyroelectric X-ray generators and a Silicon Drift Detector to conduct X-Ray Fluorescence spectroscopy (XRF) on the Moon to measure major elements: Mg, Al, Si, Ca, Ti, and Fe; minor elements: Na, K, F, S, Cr and Mn; and the trace element Ni depending on their concentration. Some factors such as roughness, grain size and porosity of sample, and the geometry of X-ray incidence, emission and energy will affect the XRF measurements precision. Basic studies on the XRF are required to develop the AXS. In this study, fused samples were used to make homogeneous samples free from the effect of grain size and porosity. Experimental and numerical studies on the XRF were conducted to evaluate the effects from incidence and emission angles and surface roughness. Angle geometry and surface roughness will be optimized for the design of the AXS on future missions from the results of the experiment and the numerical simulation. (C) 2015 Elsevier B.V. All rights reserved.
引用
收藏
页码:182 / 187
页数:6
相关论文
共 50 条
  • [1] Lunar x-ray spectrometer experiment on the SELENE mission
    Okada, T
    Kato, M
    Yamashita, Y
    Shirai, K
    Yamamoto, Y
    Matsuda, T
    Tsunemi, H
    Kitamoto, S
    LUNAR EXPLORATION 2000, 2002, 30 (08): : 1909 - 1914
  • [2] X-ray spectrometer for the Clark mission
    Catholic Univ of America, Washington, United States
    Acta Astronaut, 1-4 (293-301):
  • [3] The X-Ray Spectrometer for the Clark mission
    Starr, R
    Acuna, M
    Dennis, B
    Desai, U
    Orwig, L
    Trombka, J
    Douglass, D
    Houser, J
    Panetta, P
    Plummer, T
    Scheifele, J
    Uribe, P
    ACTA ASTRONAUTICA, 1996, 39 (1-4) : 293 - 301
  • [4] CURRENT STATUS OF DEVELOPMENT FOR ACTIVE X-RAY FLUORESCENCE SPECTROMETER FOR FUTURE PLANETARY MISSIONS.
    Nagaoka, H.
    Hasebe, N.
    Kusano, H.
    Naito, M.
    Shibamura, E.
    Kuno, H.
    Kim, K. J.
    Lopes, J. A. M.
    Martinez-Frias, J.
    METEORITICS & PLANETARY SCIENCE, 2015, 50
  • [5] First Indian lunar mission and X-ray spectrometry
    不详
    X-RAY SPECTROMETRY, 2009, 38 (01) : 75 - 75
  • [6] Numerical estimation of lunar X-ray emission for X-ray spectrometer onboard SELENE
    Ogawa, Kazunori
    Okada, Tatsuaki
    Shirai, Kei
    Kato, Manabu
    EARTH PLANETS AND SPACE, 2008, 60 (04): : 283 - 292
  • [7] Numerical estimation of lunar X-ray emission for X-ray spectrometer onboard SELENE
    Kazunori Ogawa
    Tatsuaki Okada
    Kei Shirai
    Manabu Kato
    Earth, Planets and Space, 2008, 60 : 283 - 292
  • [8] Basic studies on x-ray fluorescence analysis for active x-ray spectrometer on SELENE-2
    Kusano, Hiroki
    Hasebe, Nobuyuki
    Nagaoka, Hiroshi
    Kodama, Takuro
    Oyama, Yuki
    Tanaka, Reiko
    Amano, Yoshiharu
    Kim, Kyeong J.
    Matias Lopes, Jose A.
    HARD X-RAY, GAMMA-RAY, AND NEUTRON DETECTOR PHYSICS XV, 2013, 8852
  • [9] Wide field imaging spectrometer for ESA's future X-ray mission:: XEUS
    Strüder, L
    NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 1999, 436 (1-2): : 53 - 67
  • [10] Wide field imaging spectrometer for ESA's future X-ray mission:: XEUS
    Strüder, L
    Hartmann, R
    Holl, P
    Kemmer, J
    Klein, P
    Krause, N
    Lechner, P
    Lutz, G
    Meidinger, N
    Pfeffermann, E
    Popp, M
    Richter, R
    Soltau, H
    Trümper, J
    von Zanthier, C
    X-RAY OPTICS, INSTRUMENTS, AND MISSIONS II, 1999, 3766 : 127 - 143