Physical calibration of the LEND space-based neutron telescope: the sensitivity and the angular resolution

被引:3
作者
Mitrofanov, I. G. [1 ]
Fedosov, F. S. [1 ]
Sanin, A. B. [1 ]
Bakhtin, B. N. [1 ]
Boynton, W. [2 ]
Vostrukhin, A. A. [1 ]
Golovin, D. V. [1 ]
Kosyrev, A. S. [1 ]
Litvak, M. L. [1 ]
Malakhov, A. V. [1 ]
McClanahan, T. [3 ]
Mokrousov, M. I. [1 ]
Nuzhdin, I. O. [1 ]
Starr, R. [4 ]
Tretyakov, V. I. [1 ]
Shvetsov, V. N. [5 ]
Shevchenko, V. V. [6 ]
Harshman, K. [2 ]
机构
[1] Russian Acad Sci, Inst Space Res, Ul Profsoyuznaya 84-32, Moscow 117997, Russia
[2] Univ Arizona, Tucson, AZ USA
[3] NASA, Goddard Space Flight Ctr, Greenbelt, MD USA
[4] Catholic Univ Amer, Washington, DC 20064 USA
[5] Joint Inst Nucl Res, Ul Joliot Curie 6, Dubna 141980, Moscow Oblast, Russia
[6] Moscow MV Lomonosov State Univ, Sternberg State Astron Inst, Univ Skii Pr 13, Moscow 119899, Russia
基金
俄罗斯科学基金会;
关键词
LUNAR RECONNAISSANCE ORBITER; MARS ODYSSEY; WATER ICE; HYDROGEN; DETECTOR; EMISSION; SURFACE; POLE;
D O I
10.1134/S0020441216040096
中图分类号
T [工业技术];
学科分类号
08 ;
摘要
Results of physical calibrations of the LEND neutron telescope operating on board the NASA's LRO lunar satellite since June 2009 are described. The main goal of the LEND telescope is to measure the epithermal neutron flux in polar areas of the lunar surface with a high (similar to 10 km) resolution with the aim of determining the hydrogen distribution in the lunar regolith and detect the presence of water ice beds at the bottom of permanently shadowed lunar polar craters. The neutron detection efficiency and the effective area of the LEND detectors is experimentally estimated.
引用
收藏
页码:578 / 591
页数:14
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