共查询到18条相似文献，搜索用时 140 毫秒
1.
本文阐述了用超热中子活化分析测定矿石样品中金时，由于超热中子自屏蔽产生的金的减低情况，制备了３种不同金粒度范围的合成金矿样，并分别用热中子活化分析方法和超热中子活化方法分析。３种金粒度的范围即≤５３μｍ、５３－１５０μｍ和１５０－２５０μｍ合成的矿样，超热中子活化分析结果与热中子活化分析法比较，金分别降低了１１％、３１％和３３％，同时测量金的标准参考矿物ＭＡ－１的减低因子为５％，加拿大ＣＡＮＭＥＴ 相似文献
2.
铁基样品中锰的中子活化法测定 总被引：1，自引：0，他引：1
采用热中子与超热中子照射相结合的中子活化法测定了铁高含量样品中锰的含量。实验测定和理论计算了铁对锰的干扰系数，两者符合较好。对几个标准物质的分析结果与推荐值相符。该方法适用于ｍＦｅ／ｍＭｎ小于２×１０５的样品中锰含量的测定 相似文献
3.
水灰岩地层中子随能量和时间分布的Monte Carlo模拟 总被引：3，自引：2，他引：3
作者在MCNP的基础上，开发了中子测井，中子通量随空间、能量、时间分布蒙特卡罗（Monte Carlo)模拟软件包。对裸眼井、井眼里无下井仪器、水饱和灰岩地层、井眼注水，用该软件计算了沿井轴和沿井壁中子能量随能量、时间分布，以及沿井轴和沿井壁热中子和超热中子时间谱。即源距离变化对中子能量随能量、时间分布和井轴与井壁热中子、超热中子时间谱的影响。 相似文献
4.
介绍了热中子热井的试验原理及野外和室内试验方法，阐述了热中子测井对在含水层中运移复杂的不混溶相有机污染物探测和监测有可行性及其优缺点。 相似文献
5.
研究了微堆中子活化分析测定地质样品中卤素元素的测量条件和测量中的影响因素，对超热中子活化分析测定Ｉ和Ｂｒ进行了实验研究，Ｆ，Ｃｌ，Ｂｒ，Ｉ的检出限分别为１０＾－３、７４×１０＾－６，１．７×１０＾－６，７．８×１０＾－６。ＲＳＤ〈１５％。 相似文献
6.
水灰炭地层各孔隙度中子随能量时间分布MonteCarlo模拟 总被引：1，自引：1，他引：1
作者在MCNP的基础上，开发了中子测井，中子通量随能量、时间分布蒙特卡罗（MC）模拟软件包，对裸眼井、井眼里无下井仪器、淡水饱和灰岩地层、井眼注淡水，用该软件计算了井轴和井壁一确定点,各孔隙度中子量通量，时间分布。即孔隙度对中子通量随量、时间分布和热中子、超热中子时间谱的影响。 相似文献
7.
中子活化法测定铝材料中杂质元素 总被引：2，自引：0，他引：2
测定了用作反应堆的铝材料中Ｆｅ，Ｃｕ，Ｚｎ，Ｌａ，Ｓｍ，Ｍｏ，Ｈｆ等２３种杂质元素含量。对于Ｔｉ和Ｎｉ采用超热中子活化法，其它元素采用热中子活化法。实验测得了裂变系数，用于扣除Ｕ对Ｃｅ，Ｎｄ，Ｚｒ，Ｌａ，Ｓｍ等元素的干扰，计算了铝材中各杂质元素的探测极限，该方法精密度，对几个标准参考物质的分析结果与推荐值相符。 相似文献
8.
支霞臣 《矿物岩石地球化学通报》1988,(1)
美国麻省理工学院(MIT)地球、大气和行星科学系拥有一间专门分析地球化学样品的中子活化分析实验室。该室设备精良,组织有序,效率极高。核反应堆:MIT拥有一座研究用核反应堆(MITR—11),它为中子活化分析提供了极其方便的条件。用于分析的地质样品、岩石矿物粉末通常在核反应堆里照射6—8小时,热中子通量为4×10~(12)中子/cm~2·S。样品装在称为“Lazy Susan”的转盘中,它以每秒钟一周速度转动,以保证照射不同样品 相似文献
9.
水力压裂是提高非常规油气开采的重要手段,支撑剂位置及裂缝参数是评价压裂效果的重要因素.提出了以Gd作为示踪剂探测热中子来评价井周裂缝方法,将热中子双组扩散理论与数值模拟方法相结合,定义热中子变化参数WTN来指示裂缝宽度,并分析了岩性、井眼尺寸、地层孔隙度、地层水矿化度及含油饱和度对WTN的影响.模拟结果表明:随着裂缝宽度的增加,WTN先呈指数增加后趋于平缓;而地层孔隙度越大、地层水矿化度越小,WTN越大;井眼尺寸和地层含油饱和度的变化对WTN影响较小.利用蒙特卡罗方法建立了地层孔隙度、矿化度石灰岩地层压裂前后的数值计算模型,模拟研究了不同深度地层的热中子分布,得到了近远探测器热中子计数FAR、NEAR和WTN的响应曲线,最终处理裂缝参数结果与设定模型相吻合,验证了利用Gd示踪热中子探测方法可以来评价井周裂缝. 相似文献
10.
空气钻井条件下中子孔隙度测井响应的蒙特卡罗模拟 总被引：1，自引：0，他引：1
空气钻井作为一种欠平衡钻井技术,会对中子孔隙度测井产生不同的影响。利用蒙特卡罗方法建立裸眼井的中子孔隙度计算模型,模拟空气钻井时不同孔隙度、岩性、泥质含量、井眼尺寸、井筒空气压力条件下的中子输运过程,研究热中子计数比值与孔隙度的关系。认为空气钻井时远近探测器的热中子计数都随孔隙度的增加而增加,然后再缓慢减少;石灰岩地层的热中子计数率比值高于砂岩,泥质含量越高的地层热中子计数率比值越大;井眼尺寸对热中子计数率比值影响很大,孔隙度越大的地层井眼尺寸影响越大,且井眼尺寸越大,比值变化越小,越不利于中子孔隙度的确定;井筒空气的压力大小对热中子计数率比值影响很小。因此空气钻井时必须重新刻度中子孔隙度,并对岩性、泥质含量、井眼尺寸等因素进行校正。 相似文献
11.
I. A. Kondratyev S. G. Moiseenko G. S. Bisnovatyi-Kogan M. V. Glushikhina 《Astronomy Reports》2020,64(3):226-243
The results of three-dimensional numerical simulation of heat transfer in the outer layers of magnetized neutron stars are presented. Determining the structure of the magnetic field on a neutron star surface is an important task of modern astrophysics. In the presence of strong magnetic fields, the medium becomes anisotropic, and the laws of heat conduction change. The tensor coefficient of thermal conductivity for magnetized degenerate plasma was obtained by Bisnovatyi-Kogan and Glushikhina by solving the Boltzmann equation with the Chapman–Enskog method. In this paper, the temperature distribution on the surface of a magnetized neutron star is obtained for magnetic fields of the dipolar and quadrupolar type, as well as for their superposition. To numerically solve the stationary temperature distribution problem in the outer layers of a magnetized neutron star, the basic (support) operator numerical method was extended to a three-dimensional case. The problem was solved on the grid which consists of tetrahedra. 相似文献
12.
《International Geology Review》2012,54(1):11-16
The reaction of minerals of boron to neutron radiation; is such that neutron logging of boreholes provides a geophysical tool with which to seek their ores.. It is based on the reaction of the isotope of boron B1O with a thermal neutron: B10 + n9 → Li7 + α. A sonde designed specifically for the purpose has been tested. Until they are generally available, another type can easily he modified for neutron logging of boron. Different procedures and interpretation permit initial identification, preliminary assay, and estimates of reserves. —M. Russell 相似文献
13.
N.W. BOWER E.S. GLADNEY R.C. HAGAN P.E. TRUJILLO R.G. WARREN 《Geostandards and Geoanalytical Research》1985,9(2):199-203
Data on three Japanese geochemical reference samples (JR-1, JA-1, and JB-2) are presented. Ten major and thirty-five trace element concentrations were determined using x-ray fluorescence, instrumental thermal neutron activation, thermal neutron capture prompt gamma-ray spectrometry, delayed neutron assay, automated thermal neutron activation analysis, inductively coupled plasma emission, atomic absorption, and ion selective electrode. Good agreement between the various methods and with recent literature values were obtained using error weighted mean concentrations for the samples. 相似文献
14.
C.M Hohenberg 《Geochimica et cosmochimica acta》1981,45(2):251-256
Parameters for a number of neutron irradiations are examined and results intercompared for the Bjurböle meteorite; data for the 1967 Valecitos-1 irradiation are presented. Apparent I-Xe ‘formation’ ages are reproducible for three different samples of Bjurböle, suggesting isotopic homogeneity for initial iodine in the bulk material. The systematics of neutron capture in 135Xe (produced from 235U neutron fission) are examined and verified in irradiated BCR-1. 相似文献
15.
介绍了地—空界面天然中子流的来源和轻便型天然中子流测量仪器。论述了地—空界面天然中子辐射场的扰动。理论与长期观测表明,在地—空界面上天然中子流注量率随高程的增加而呈指数规律增加,而在近地表(20m内)却随距地面高度的增加而呈指数规律减少;天然中子流注量率与大气压力呈负相关关系,气压系数为(-0.060～-0.064)中子计数/30min/kPa;地—空界面天然中子流的纬度效应与高空中更显著;天然中子流注量率异常与气象的变化密切相关;地表介质的含水率增高,则地—空界面上升快中子流明显降低。通过对地一空界面天然中子流测量,可以揭示气象的瞬态变化、确定地表介质的含水率的关系,以及在地震预报与环境电离辐射评价方面具有重要的科学意义与实用价值。 相似文献
16.
We explore the possibility of explaining Anomalous X-ray Pulsars (AXPs) and Soft Gammaray Repeaters (SGRs) in a scenario with fall-back magnetic accretion onto a young isolated neutron star. The X-ray emission of the pulsar in this case originates due to the accretion of matter onto the surface of the neutron star from a magnetic slab surrounding its magnetosphere. The spin-down rate of the neutron star expected in this picture is close to the observed value. We show that such neutron stars are relatively young and are going through the transition from the propeller state to the accretor state. The pulsar’s activity in gamma-rays is connected with its relative youth, and is enabled by energy stored in a non-equilibrium layer located in the crust of the low-mass neutron star. This energy can be released due to the mixing of matter in the neutron star crust with super heavy nuclei approaching its surface and becoming unstable. The fission of nuclei in the low-density region initiates chain reactions leading to a nuclear explosion. Outbursts are probably triggered by instability developing in the region where the matter accreted by the neutron star accumulates in the magnetic polar regions. 相似文献
17.
本文讨论了利用低强度中子源在萤石矿进行中子活化测井的测量技术问题，以及资料的处理方法和解释，并用实测结果验证了利用低强度源进行中子活化测井的可行性和有效性。 相似文献
18.
Assuming that the observed periodic variations of pulsar emission are due to the free precession of the spin axis, we investigate the evolution of the rotation of a two-layer neutron star using the Hamiltonian method of Getino. We model the dynamical characteristics of a rotating neutron star using the observed variations of the emission of seven pulsars. We estimate the dependence of the period of the Chandler wobble, the period of precession of the spin axis, and the dynamical ellipticity of a neutron star on the model used to describe the super-dense neutron matter and the mass of the star. 相似文献