Wilson Jody K, Spence Harlan E, Schwadron Nathan A, Case Anthony W, Looper Mark D, Jordan Andrew P, de Wet Wouter, Kasper Justin
Institute for the Study of Earth, Oceans, and Space, University of New Hampshire, Durham, NH, USA.
Solar System Exploration Research Virtual Institute, NASA Ames Research Center, Moffet Field, California, USA.
Geophys Res Lett. 2020 Jan 16;47(1). doi: 10.1029/2019gl085522. Epub 2020 Dec 23.
We have invented a new method for detecting solar particle events using data from the Cosmic Ray Telescope for the Effects of Radiation (CRaTER) on the Lunar Reconnaissance Orbiter (LRO). Using a simple function of the total particle detection rates from four of CRaTER's six detectors, we can precisely identify solar energetic particle event periods in the CRaTER data archive. During solar-quiet periods we map the distribution of a mare-associated mixture of elements in the lunar regolith using this new method. The new map of the moon probably reflects an as-yet unknown combination of lunar albedo protons, neutrons, and gamma rays, and most closely resembles Lunar Prospector maps of gamma rays characteristic of thorium and iron. This result will lead to multiple follow-up studies of lunar albedo particles and may also contribute to the study of diurnally-varying hydrogenation of the lunar regolith.
我们发明了一种利用月球勘测轨道飞行器(LRO)上的宇宙射线辐射效应望远镜(CRaTER)的数据来探测太阳粒子事件的新方法。通过使用CRaTER六个探测器中四个的总粒子探测率的简单函数,我们可以精确识别CRaTER数据档案中的太阳高能粒子事件周期。在太阳平静时期,我们使用这种新方法绘制月球风化层中与月海相关的元素混合物的分布图。新的月球地图可能反映了月球反照率质子、中子和伽马射线的一种尚未知晓的组合,并且与钍和铁特征的伽马射线的月球勘探者地图最为相似。这一结果将引发对月球反照率粒子的多项后续研究,也可能有助于对月球风化层日变化氢化作用的研究。