|
|
|
|
|
|
Researchon the Selection of Mars Onboard Laser Induced Breakdown Spectrometer (MarsCoDe) Calibration Samples |
CAI Ting-ni1,2, LI Chun-lai1*, REN Xin1, LIU Bin1, LIU Da-wei1 |
1. Key Laboratory of Lunar and Deep Space Exploration, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
2. School of Physical and Science, University of Chinese Academy of Sciences, Beijing 100049, China |
|
|
Abstract The first Mars Global remote sensing and regional survey mission of China has been approved for the first time, and the first Mars probe is going to Mars. In order to meet the needs of Mars material composition analysis, different types of instruments on Mars rover have been developed in China, including Mars Surface composition detection Package (MarsCoDe) using laser-induced breakdown spectroscopy (LIBS) technology. Because the surface of Mars is covered with dust, we must get rid of the dust layer or destroy rock surface if we want to detect the material composition under the Mars dust accurately. LIBS can be used to ablate the surface of the object by its laser, and obtain the spectral information of deep rock. In addition, LIBS is almost suitable for detecting every element in Mars exploration, including light elements H, Li, Be, B, C, N, O, etc., which helps to find evidence for organic matter and water-bearing geological process. Due to Mars environment, the physical properties of the plasma are completely different from those on earth. In order to ensure the quality of the returned LIBS spectral data, it is necessary to carry out onboard calibration after landing, meanwhile carrying calibration board with specific standard samples on Mars rover, for data correction, ensuring the reliability of the returned data and more accurately interpreting the Martian surface material. The selection of calibration samples is a very important work. There are various factors such as the limitation of equipment engineering conditions, the representativeness of the calibration sample types, the distribution range of the elements and the stability of the samples. In this paper, we summarized the research progress of onboard calibration of Mars onboard LIBS and focused on analyzing the selection criteria of LIBS calibration samples and the advantages and disadvantages of foreign sample selection. After summarizing experiences, some suggestions were put forward to provide reference for our onboard calibration work. This article is of scientific significance to the correct interpretation of Mars exploration data and future research on the origin of Mars and the long-term geological evolution of Mars.
|
Received: 2018-03-14
Accepted: 2018-08-15
|
|
Corresponding Authors:
LI Chun-lai
E-mail: licl@nao.cas.cn
|
|
[1] Allwood A. Spectroscopy, 2015, 30(7): 22.
[2] Chevrier V, Mathé P E. Planetary and Space Science, 2007, 55(3): 289.
[3] Ming D W, Gellert R, Morris R V, et al. Journal of Geophysical Research Atmospheres, 2008, 113: 1029.
[4] Campbell J L, King P L, Burkemper L, et al. Nuclear Instruments & Methods in Physics Research, 2014, 323(3): 49.
[5] Blake D F, Vaniman D T, Yen A S, et al. Mineralogical Capabilities of the CheMin XRD/XRF Instrument on Mars Science Laboratory(MSL’11). AGU Fall Meeting, 2009. 43A.
[6] Wiens R C, Maurice S, Barraclough B, et al. Space Science Reviews, 2012, 170(1-4): 167.
[7] Jackson R S, Wiens R C, Vaniman D T, et al. Icarus, 2016, 277: 330.
[8] Maurice. S, Wiens R C, Mouélic S L, et al. The SuperCam Instrument for the Mars2020 Rover. European Planetary Science Congress, 2015, 10.
[9] Maurice S, Wiens R C, Saccoccio M, et al. Space Science Reviews, 2012, 170(1-4): 95.
[10] Melikechi N, Mezzacappa A, Cousin A. Spectrochimica Acta Part B Atomic Spectroscopy, 2014, 96(6): 51.
[11] Fabre C, Cousin A, Wiens R C, et al. Spectrochimica Acta Part B: Atomic Spectroscopy, 2014, 99: 34.
[12] Maurice S, Clegg S M, Wiens R C, et al. Journal of Analytical Atomic Spectrometry, 2016, 31(4): 863.
[13] Forni O, Maurice S, Gasnault O, et al. Spectrochimica Acta Part B: Atomic Spectroscopy, 2013, 86: 31.
[14] Clegg S M, Wiens R C, Anderson R, et al. Spectrochimica Acta Part B: Atomic Spectroscopy, 2017, 129: 64.
[15] Wiens R C, Maurice S, Lasue J. Spectrochimica Acta Part B: Atomic Spectroscopy, 2013, 82: 1.
[16] Lanza N L, Wiens R C, Clegg S M, et al. Applied Optics, 2010, 49(13): C211.
[17] Vaniman D, Dyar M D, Wiens R, et al. Space Science Reviews, 2012, 170(1-4): 229.
[18] Cousin A, Forni O, Maurice S. Spectrochimica Acta Part B: Atomic Spectroscopy, 2011, 66(11/12): 805.
[19] Unnikrishnan V K, Mridul K, Nayak R, et al. Pramana, Journal of Physics, 2012, 79(2): 299.
[20] Boucher T F, Ozanne M V, Carmosino M L, et al. Spectrochimica Acta Part B: Atomic Spectroscopy, 2015, 107: 1.
[21] Dyar M D, Carmosino M L, Breves E A. Spectrochimica Acta Part B: Atomic Spectroscopy, 2012, 70: 51.
[22] Anderson R B, Morris R V, Clegg S M, et al. Icarus, 2011, 215(2): 608.
[23] Forni O, Maurice S, Gasnault O. Spectrochimica Acta Part B: Atomic Spectroscopy, 2013, 86: 31.
[24] Fabre C, Maurice S, Cousin A, et al. Spectrochimica Acta Part B: Atomic Spectroscopy, 2011, 66(3-4): 280.
[25] Rapin W, Meslin P Y, Maurice S, et al. Earth and Planetary Science Letters, 2016, 452: 197.
[26] Schroeder S, Meslin P Y, Gasnault O, et al. Icarus, 2015, 249: 43.
[27] Lanza N L A, Ollila A M B, Cousin A A, et al. Icarus, 2015, 249(SI): 62.
[28] Nachon M, Clegg S M, Mangold N, et al. Journal of Geophysical Research: Planets, 2014, 119(9): 1991.
[29] Cousin A, Sautter V, Fabre C, et al. Journal of Geophysical Research: Planets, 2012, 117(E10): e10001.
[30] Cousin A, Sautter V, Payre V, et al. Icarus, 2017, 288: 265.
[31] Fabre C, Maurice S, Cousin A. Spectrochimica Acta Part B: Atomic Spectroscopy, 2011, 66(3-4): 280.
[32] Rapin W, Meslin P Y, Maurice S, et al. Spectrochimica Acta Part B: Atomic Spectroscopy, 2017, 130: 82. |
[1] |
BAO Pei-jin1, CHEN Quan-li1, 3*, ZHAO An-di1, REN Yue-nan2. Identification of the Origin of Bluish White Nephrite Based on
Laser-Induced Breakdown Spectroscopy and Artificial
Neural Network Model[J]. SPECTROSCOPY AND SPECTRAL ANALYSIS, 2023, 43(01): 25-30. |
[2] |
XU Jin-li1, 2, HU Meng-ying1, 2, ZHANG Peng-peng1, 2, XING Xia1, 2, BAI Jin-feng1, 2, ZHANG Qin1, 2*. Application of High Pressure Pelletised Sample and LIBS in the Determination of Rare Earth Elements in Soil Samples[J]. SPECTROSCOPY AND SPECTRAL ANALYSIS, 2020, 40(12): 3806-3811. |
[3] |
CHEN Xing-feng1, 2, LIU Li3*, GE Shu-le3, LI Xin4, ZHANG Kai-nan2, YANG Ben-yong4. Research Progress for In-Flight Calibration of the Large View Polarized Multispectral Camera[J]. SPECTROSCOPY AND SPECTRAL ANALYSIS, 2020, 40(02): 343-349. |
[4] |
FU Li-ping1,2, JIA Nan1, 2,3, HU Xiu-qing4*, MAO Tian4, JIANG Fang1,2, WANG Yun-gang4, PENG Ru-yi1,2, WANG Tian-fang1,2,3, WANG Da-xin3, DOU Shuang-tuan3. Research Progress on On-Orbit Calibration Technology for Far Ultraviolet Payload[J]. SPECTROSCOPY AND SPECTRAL ANALYSIS, 2019, 39(12): 3673-3680. |
[5] |
HONG Guang-lie1, ZHOU Yan-bo1,2, LIU Hao1, KONG Wei1, SHU Rong1,2*. Feasibility Study of Mars Rover’s Laser Induced Breakdown Spectroscopy Based Mie-Lidar Design[J]. SPECTROSCOPY AND SPECTRAL ANALYSIS, 2018, 38(02): 600-605. |
[6] |
ZHAO Wei-ning1, 2, FANG Wei2, JIANG Ming2, LUO Yang2, WANG Yu-peng2* . Overview of the Study for Transfer Radiometer with Spectral Standard Calibration and Transferring Technology [J]. SPECTROSCOPY AND SPECTRAL ANALYSIS, 2016, 36(09): 2984-2990. |
[7] |
LIU Yi1,2, YIN Da-yi1 . Study on In-Orbit VIS/SWIR Relative Calibration Monitoring System with High Stability [J]. SPECTROSCOPY AND SPECTRAL ANALYSIS, 2014, 34(04): 927-931. |
[8] |
YAO Ning-juan,CHEN Ji-wen,YANG Zhi-jun,WANG Hai-zhou. Laser-Induced Breakdown Spectrometer——A New Tool for Quick Analysis of On-the-Spot Sample in Metallurgy[J]. SPECTROSCOPY AND SPECTRAL ANALYSIS, 2007, 27(07): 1452-1454. |
|
|
|
|