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Optically stimulated luminescence (OSL) study of synthetic stishovite

机译:合成硅钙石的光激发发光(OSL)研究

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Optically stimulated luminescence (OSL) of synthetic stishovite was investigated for a future dating technique of meteor impact craters. Luminescence around 330 nm was measured on the gamma -ray irradiated stishovite under two stimulating light sources of infrared laser (830 nm) and blue light emitting diode set (470 nm). Thermoluminescence (TL) studies before and after the OSL measurements showed the intensities around 100-200 degreesC and 220-350 degreesC to increase and those around 350-450 degreesC to decrease. This indicates that a part of deep-trapped charges excited during the OSL measurements were retrapped by shallower traps. The infrared stimulated luminescence (IRSL) after the TL measurement up to 450 degreesC could not be detected, while the blue light stimulated luminescence (BLSL) after TL had about one-tenth of the intensity before TL, This indicates that a part of the charges in shallower traps were detrapped thermally and returned to the deeper traps which were related to BLSL, The result implies that some of the BLSL-related traps are quite stable at room temperature and could be used for geological dating. In addition, two paramagnetic centers produced by sudden release of high pressure in synthesis process were found in the unirradiated stishovite by electron spin resonance (ESR). Their g-factors are g(parallel to) = 2.00181 and g(perpendicular to) = 2.00062 for an axial signal and g = 2.00305 for the other isotropic signal. These signals could be used for an evidence of impacts if those signals could be stored in geological time. (C) 2000 Elsevier Science Ltd. All rights reserved. [References: 20]
机译:研究了合成的人造钛矿的光激发发光(OSL),以用于流星撞击坑的未来测年技术。在红外激光(830 nm)和蓝色发光二极管组(470 nm)的两个刺激光源下,在经γ射线照射的辉石上测量了330 nm附近的发光。 OSL测量前后的热致发光(TL)研究表明,在100-200摄氏度和220-350摄氏度附近的强度增加,而在350-450摄氏度附近的强度降低。这表明在OSL测量期间激发的一部分深陷电荷被较浅的陷阱重新捕获。在TL测量至450摄氏度时,无法检测到红外激发发光(IRSL),而TL之后的蓝光激发发光(BLSL)具有TL之前强度的十分之一,这表明部分电荷在较浅的圈闭中进行热圈闭并返回到与BLSL有关的较深圈闭,结果表明某些与BLSL相关的圈闭在室温下相当稳定,可用于地质定年。此外,在未辐照的辉石中,通过电子自旋共振(ESR)在合成过程中发现了由高压突然释放而产生的两个顺磁中心。对于轴向信号,它们的g因子为g(平行)= 2.00181,对于垂直信号,它们的g(垂直于)= 2.00062,对于其他各向同性信号,它们的g = 2.00305。如果这些信号可以在地质时间内存储,则这些信号可以用作影响的证据。 (C)2000 Elsevier ScienceLtd。保留所有权利。 [参考:20]

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