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首页> 外文期刊>Radiation measurements >On the frequency distributions per unit area of the projected and etchable lengths of surface-intersecting fission tracks: influences of track revelation, observation and measurement
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On the frequency distributions per unit area of the projected and etchable lengths of surface-intersecting fission tracks: influences of track revelation, observation and measurement

机译:关于表面相交裂变径迹的可投影长度和可蚀刻长度的每单位面积的频率分布:径迹揭示,观测和测量的影响

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摘要

In addition to the statistical bounds discussed by Laslett et ar. (1994) and Laslett and Galbraith (1996), thermal history analysis based on the projected and etchable length distributions of surface intersecting fission tracks is limited by systematic factors related to track revelation, observation and measurement. The effects of track revelation, in particular, distort these distributions in the length intervals of interest. An observation threshold poses a problem if it is described by a critical angle theta(c), but not if it is described by other criteria proposed in the literature. Measurement imprecisions, predictably, blur the thermal history information contained in these distributions. Measurements of semi-confined tracks, added as a result of surface etching, are a more promising alternative to confined track length measurements for accessing the thermal history record in the fission track length distribution. On the other hand, measurements of the projected lengths of surface intersecting tracks offer the theoretical possibility of determining the true volumetric density N and true mean length m of an arbitrary population of fission tracks, thus allowing direct determination of the corrected age: of samples with complex thermal histories. On a methodical level, knowledge of N and m allows to determine the efficiency with which fission tracks are counted under the optical microscope under exactly the same conditions as those under which fission track counts for routine dating purposes are performed. (C) 1999 Elsevier Science Ltd. All rights reserved. [References: 26]
机译:除了Laslett等人讨论的统计界限外。 (1994)以及Laslett和Galbraith(1996),基于表面相交裂变径迹的预计和可蚀刻长度分布的热历史分析受到与径迹揭示,观测和测量相关的系统因素的限制。轨道揭示的影响尤其会在感兴趣的长度间隔中扭曲这些分布。如果用临界角theta(c)描述观察阈值,则会带来问题,但如果用文献中提出的其他标准描述观察阈值,则不会出现问题。可以预见的是,测量误差会模糊这些分布中包含的热历史信息。作为表面蚀刻的结果而添加的半封闭磁道的测量,对于访问裂变磁道长度分布中的热历史记录的局限磁道长度测量而言,是一种更有希望的替代方法。另一方面,测量表面相交轨道的投影长度可以为确定任意裂变轨道群的真实体积密度N和真实平均长度m提供理论上的可能性,从而可以直接确定校正后的年龄:复杂的热历史。从方法上讲,N和m的知识可以确定在光学显微镜下与进行常规测年目的裂变径计数的条件完全相同的条件下,对裂变径进行计数的效率。 (C)1999 Elsevier ScienceLtd。保留所有权利。 [参考:26]

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