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Journal ArticleDOI

Instrument Calibrations and Data Analysis Procedures for the NEAR X-Ray Spectrometer

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TLDR
The X-ray spectrometer onboard the Near Earth Asteroid Rendezvous spacecraft will measure X-rays from the surface of 433 Eros in the energy region 0.7-10 keV as discussed by the authors.
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This article is published in Icarus.The article was published on 2000-10-01. It has received 28 citations till now. The article focuses on the topics: Spectrometer.

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Elemental Composition of 433 Eros: New Calibration of the NEAR-Shoemaker XRS Data

TL;DR: In this article, a new calibration of the elemental-abundance data for Asteroid 433 Eros taken by the X-ray spectrometer (XRS) aboard the NEAR-Shoemaker spacecraft is presented.
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Minor element evidence that Asteroid 433 Eros is a space-weathered ordinary chondrite parent body

TL;DR: Cheng et al. as discussed by the authors reported that 433 Eros is a primitive body with composition and mineralogy similar to ordinary chondrites, but with a surface heavily modified by interactions with the solar wind and micrometeorites, processes collectively termed space weathering.
References
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Radiation detection and measurement

TL;DR: In this paper, the authors present a detailed analysis of the effect of different types of detectors on the performance of the detection of neutrons and their effect on the detection efficiency and error prediction.
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Apollo 15 Geochemical X-ray Fluorescence Experiment: Preliminary Report.

TL;DR: The results indicate the existence of a differential lunar highland crust, probably feldspathic, related to the plagioclase-rich materials previously found in the samples from Apollo 11, Apollo 12, Apollo 14, Apollo 15, and Luna 16.
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Apollo 16 geochemical x-ray fluorescence experiment: preliminary report.

TL;DR: The lunar surface was mapped with respect to magnesium, aluminum, and silicon as aluminum/ silicon and magnesium/ silicon intensity ratios along the projected ground tracks swept out by the orbiting Apollo 16 spacecraft to confirm the idea that the moon has a widespread differentiated crust (the highlands).
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Remote X-ray spectrometry for NEAR and future missions: Modeling and analyzing X-ray production from source to surface

TL;DR: In this article, the authors discuss the nature of such variations expected for missions to an asteroid, the Moon, and Mercury, and discuss an effective means of removing the effects of solar variability from surface measurements, as indicated by the agreement between theoretical models presented here and Apollo X-ray observations.
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