东亚速地区的砂矿钻石

IF 0.5 Q4 MINERALOGY
V. Kvasnytsya
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引用次数: 0

摘要

研究了东亚速地区第四纪冲积矿床中金刚石的晶体形态、光致发光行为、氮杂质浓度和拉曼光谱。来自Mius-Krynka河流域的大钻石呈现出理想的菱形十二面体结构,其几何参数与金伯利岩和煌斑岩中的圆形钻石相似。利用红外光谱、氮杂质的含量和状态以及晶体中的其他缺陷,确定了亚速金刚石形成的地幔温度状态。钻石可以分为不同的光谱类型,即IaA, iab和IIa。它们的氮含量较低,为19 ~ 491ppm,平均氮含量为148ppm,氮聚集程度较高(平均值% B = 33)。东亚速河钻石的温度测量数据在1097-1175ºC之间,持续了20亿年,晶体在地幔中停留了30亿年,温度范围为1120-1165ºС。在光致发光光谱测量中发现了N3、S1和575 nm中心。金刚石的拉曼位移在1331.0 ~ 1332.1 cm-1之间。这些钻石可能与地幔榴辉岩有关,它们是由金伯利岩带到地球表面的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
PLACER DIAMONDS OF THE EASTERN AZOV REGION
The crystal morphology, photoluminescence behavior, nitrogen impurity concentrations and Raman spectra of diamonds from Quaternary alluvial deposits of the Eastern Azov region were studied. Macrodiamond from the Mius-Krynka river basin shown ideal rhombic dodecahedron habitus, and their geometric parameters are similar to those of rounded diamonds found in kimberlites and lamproites. The mantle temperature regime for the formation of Azovian diamonds was determined using infrared spectroscopy, the content and state of nitrogen impurities, and other defects in the crystals. Diamonds can be divided into different spectral types namely IaA, IaAB and IIa. They have low nitrogen contents from 19 to 491 ppm, with an average nitrogen content of 148 ppm and they have a relatively high degree of nitrogen aggregation (average value of % B = 33). Thermometric data for the Eastern Azov diamonds are in the range of 1097-1175 ºC for 2 billion years and 1120-1165 ºС for 3 billion years of crystals to stay in the mantle. N3, S1 and 575 nm centers are revealed in the photoluminescence spectroscopic measurements. The Raman shift for diamonds is in the range of 1331.0-1332.1 cm–1. The diamonds are probably associated with mantle eclogites, and they have been brought to Earth’s surface by kimberlites.
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来源期刊
CiteScore
0.70
自引率
0.00%
发文量
18
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