Carryover of Sampling Errors and Other Problems in Far-Infrared to Far-Ultraviolet Spectra to Associated Applications

1区 地球科学 Q1 Earth and Planetary Sciences
A. Hofmeister
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引用次数: 6

Abstract

The thin, smooth curves representing spectroscopic data suggest a high degree of accuracy. Yet, experimental uncertainties do exist, as in any measurement. Overlooked problems in data collection, processing, and interpretation have repercussions for applications in mineral physics, planetary science, and astronomy. Random errors (i.e., noise) are fairly obvious, and are not discussed here. The concern is subtle and overlooked errors that arise in acquisition, processing, and interpretation of spectral data. These types of errors are systematic, not random. This chapter identifies various systematic errors and problems that the author encountered in her efforts to provide absolute values of absorbance or reflectivity. Re-occurring issues in data collection include underestimating the importance of surface polish and not accounting for peak profiles depending on sample thickness relative to band strengths. Processing of emission spectra is problematic. Common instrumental problems are briefly described. Optical spectroscopy is the name generally attached to the visible region which we probe with our eyes, which are convenient built-in spectrometers, but can also include the infrared (IR) region wherein the type of vibrational mode known as “optical” is detected. Because some applications require very high frequency (ν) data, this chapter concerns ν from ~10 to 106 wavenumbers, which is equivalent to wavelengths (λ) of ~106 to 10 nm or of ~1000 to 0.01 μm). The X-ray region is included due to the extreme breadths of metal-oxygen charge-transfer bands of minerals which peak in the ultraviolet (UV). The author points out errors in her own results as well those of others. Mistakes provide opportunity for learning! Correct methodologies are discussed along with measurements needed to improve constraints on spectral parameters and hence to make interpretations more definitive. Ideal conditions are difficult to achieve, so another goal is enable the reader to recognize what is “sufficiently accurate” and/or “representative” …
远红外到远紫外光谱采样误差的残留及其他问题在相关应用中的应用
代表光谱数据的细而光滑的曲线显示出高度的准确性。然而,实验的不确定性确实存在,就像在任何测量中一样。在数据收集、处理和解释中被忽视的问题对矿物物理学、行星科学和天文学的应用产生了影响。随机误差(即噪声)是相当明显的,这里不讨论。关注的是在光谱数据的获取、处理和解释中出现的微妙和被忽视的错误。这些类型的错误是系统性的,而不是随机的。本章确定了作者在努力提供吸光度或反射率绝对值时遇到的各种系统错误和问题。数据收集中反复出现的问题包括低估表面抛光的重要性,以及不考虑根据样品厚度相对于带强度的峰值轮廓。发射光谱的处理存在问题。简要描述了常见的仪器问题。光谱学通常是我们用眼睛探测的可见区域的名称,这是方便的内置光谱仪,但也可以包括红外(IR)区域,其中被称为“光学”的振动模式类型被检测到。由于一些应用需要非常高频率(ν)的数据,本章涉及到~10到106个波数的ν,这相当于波长(λ)在~106到10nm或~1000到0.01 μm之间。x射线区域是由于矿物的金属-氧电荷转移带的极端宽度,其在紫外线(UV)中达到峰值。作者指出了她自己和其他人的研究结果中的错误。错误是学习的机会!讨论了正确的方法以及改善光谱参数限制所需的测量,从而使解释更加明确。理想的条件很难实现,所以另一个目标是让读者认识到什么是“足够准确的”和/或“代表性的”……
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来源期刊
Reviews in Mineralogy & Geochemistry
Reviews in Mineralogy & Geochemistry 地学-地球化学与地球物理
CiteScore
8.30
自引率
0.00%
发文量
39
期刊介绍: RiMG is a series of multi-authored, soft-bound volumes containing concise reviews of the literature and advances in theoretical and/or applied mineralogy, crystallography, petrology, and geochemistry. The content of each volume consists of fully developed text which can be used for self-study, research, or as a text-book for graduate-level courses. RiMG volumes are typically produced in conjunction with a short course but can also be published without a short course. The series is jointly published by the Mineralogical Society of America (MSA) and the Geochemical Society.
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