许家窑泥河湾沉积物的岩石磁学性质

对许家窑泥河湾河湖相沉积物开展的一系列岩石磁学实验结果显示: 磁铁矿、磁赤铁矿和赤铁矿为主要的载磁矿物; 低温磁化率和低温剩磁测量是查明磁铁矿、磁赤铁矿化及超顺磁颗粒存在的非常有效的手段; 尽管在局部深度上部分磁铁矿可能经历了低温氧化, 但SD/MD磁铁矿颗粒的大量存在仍是沉积物磁化率增强的主要原因之一; SD/MD磁铁矿和赤铁矿为碎屑成因, 由二者为主要磁性载体的特征剩磁(ChRM)反映了沉积物形成时的原始磁场, 而磁赤铁矿则可能代表了叠加于原生剩磁上后生的化学成分.     

豫北早古生代灰岩的岩石磁学研究

对一些可分离出岩石形成时原生剩磁的样品进行深入的岩石磁学研究,发现天然剩磁的特征通常取决于磁铁矿的颗粒度(或单、多磁畴状态),单、多磁畴磁铁矿的含量不同,导致了中温与高温剩磁分量不同程度的叠加,也就造成了不同磁分量分离难易程度的不同     

中中新世秦安黄土-古土壤序列磁性增强机制及其环境意义

中中新世黄土高原风尘堆积序列磁化率显著增高,在区域内已成为地层对比标志,然而其磁性增强机制依然不清楚.本文对秦安地区QA-I剖面约14～17.1 Ma期间的黄土-古土壤样品进行了系统的环境磁学、岩石磁学(热磁性质、磁滞性质、非磁滞剩磁与饱和等温剩磁比值χ_ARM/SIRM等)和色度指标分析.结果表明,QA-I剖面黄土-古土壤序列样品中磁性矿物为准单畴(PSD)磁铁矿、超顺磁/单畴(SP/SD)磁赤铁矿和赤铁矿,古土壤中细粒磁赤铁矿含量高于上下相邻黄土层.CBD(Citrate-Bicarbonate-Dithionite)处理方法显示,中中新世风尘序列中碎屑成因的PSD磁铁矿含量变化不大,约14.5～16.0 Ma期间成壤成因SP/SD磁赤铁矿含量的增多,是导致该时期风尘堆积序列磁化率增强的主要原因;这与该时期较低的土壤发育程度并不一致,表明CBD处理方法虽然可有效获取成壤成因SP/SD磁赤铁矿信息,却无法区分其为当地还是源区成壤成因.低温磁学研究表明,QA-I剖面约14.5～16.0 Ma期间SP/SD磁赤铁矿可能为碎屑磁铁矿颗粒的风化外壳,其含量高低变化与风尘样...     

天山北缘新近系沉积物岩石磁学研究

岩石磁学研究表明, 天山北缘塔西河剖面新近系可划分为湖相沉积型、河流相沉积型和冲积扇沉积型三种类型, 分别对应于剖面的底部(沙湾组和塔西河组中下部)、中部(塔西河组顶部和独山子组中下部)和上部(独山子组顶部和西域组), 其中湖相沉积岩石磁学性质复杂, 除与沉积物物源密切相关外, 还可能受风化作用、原地磁性矿物自生或成岩作用以及生物活动的影响, 天然剩磁强度为10^-3~10^-2 A/m, 主要磁性矿物为磁铁矿, 高矫顽力磁性矿物可能为针铁矿. 磁性矿物颗粒由假单畴和单畴(PSD+SD)或单畴和超顺磁混合组成(SD+SP); 河流相沉积天然剩磁强度为10^-2~10^-1 A/m, 主要磁性矿物为磁铁矿和赤铁矿, 磁性矿物颗粒为假单畴(PSD), 450~580℃可获得稳定的特征剩磁方向, 特征剩磁载磁矿物为磁铁矿; 冲积扇沉积天然剩磁强度介于湖相和河流相沉积之间, 主要磁性矿物也为磁铁矿和赤铁矿, 580~680℃获得稳定特征剩磁方向, 特征剩磁载磁矿物为赤铁矿, 磁性矿物颗粒为假单畴(PSD).     

三门峡盆地晚新生代沉积物磁性载体类型

对三门峡盆地晚新生代沉积岩样品进行岩石磁学研究,通过三轴饱和等温剩磁和剩磁矫顽力实验、交变退磁和热退磁实验及磁化率测定,发现黄土-古土壤、河湖相灰绿层和冲洪积层3种不同岩性的磁载体存在显著差异.即黄土-古土壤以磁铁矿为主,赤铁矿和磁赤铁矿很少;河湖相灰绿色沉积磁性矿物含量较低,主要为赤铁矿和磁铁矿,但磁铁矿较多,此外还有一些不稳定磁性矿物(如针铁矿、菱铁矿等);冲洪积物以磁铁矿和赤铁矿为主,磁铁矿相对较多.     

华北地块早古生代地层单元的岩石磁学特征研究

通过对采自华北地块西部鄂尔多斯盆地边缘早古生代地层单元中的４４块定向岩芯样品的岩石磁学实验（饱和等温剩磁及剩磁矫顽力的测量，三轴磁化的饱和等温剩磁的系统热退磁和低温实验）研究，揭示出华北地块早古生代地层单元的各类岩石中，主要载磁矿物的构成具有磁铁矿或赤铁矿与中等居里温度的磁黄铁矿、磁赤铁矿等共存的特征；个别地层单元的岩石中以极低居里点的针铁矿为主要载磁矿物．     

有机质对纳米级磁铁矿热稳定性的影响

单畴磁铁矿颗粒是地质样品中最重要的磁性载体,其稳定性一直备受关注.为了认识有机质对纳米级磁铁矿颗粒热稳定性的影响,本文对比研究了趋磁细菌AMB-1合成的单畴磁铁矿分别在全细胞中和经去胞提纯后的纯化磁小体中的热磁性质,以及热处理后样品的磁滞参数和低温磁性的变化.发现仅有磁小体膜包裹的纯化磁小体中单畴磁铁矿热稳定性极强,而全细胞中的单畴磁铁矿加热过程中发生了显著的热变化:磁铁矿在约270℃即开始转化,400℃以前几乎完全被有机质还原为顺磁性物质;同时在400℃以前,有机质的还原作用与有机质热分解引起磁小体链的坍塌,共同导致了样品矫顽力(B_c)、剩磁矫顽力(B_cr)和剩磁比(M_rs/M_s)的减小,以及矫顽力比(B_cr/B_c)的增加. 我们的实验结果清楚地表明,当地质样品中含有较多有机质组分并受热事件影响时,其中的单畴磁铁矿难以得到保存.     

四川旺苍地区中三叠世雷口坡组重磁化机理初步研究

对四川北部旺苍地区中三叠世雷口坡组进行了古地磁学和岩石磁学研究,结果表明,主要载磁矿物为多畴磁铁矿和磁赤铁矿,所携带的特征剩磁在地理坐标下与近代地磁场方向接近,可能是由于后期白云岩化作用和热粘滞剩磁引起的重磁化所致.     

华北盆地南缘早古生代岩石的重磁化——Ⅱ.岩石磁学结果

华北盆地南缘早古生代岩石系统的岩石磁学研究表明,其岩石中的磁性矿物组合相当复杂,重磁化时代可分为晚二叠/早三叠世和早、晚白垩世2个大的阶段.焦作剖面具有原生剩磁和次生剩磁岩石共生的特征,以及细致的岩石磁学分析表明,未重磁化和重磁化岩石两者间磁铁矿颗粒度大小存在明显区别,这暗示了热粘滞剩磁是重磁化的重要原因之一,而济源和登封剖面不仅岩石遭受完全的重磁化,而且广泛发育早白垩时期形成的磁黄铁矿,磁黄铁矿形成则暗示着造山热液的渗透作用.     

黄土高原西北缘末次冰期晚期以来黄土沉积物的岩石磁学性质

以黄土高原西北缘的靖远和古浪剖面(包含黄土层L1上部和占土壤层SO)作为研究对象,选取代表性样品进行磁化率、频率磁化率、热磁曲线、等温剩磁获得曲线和磁滞回线等测定.结果表明,靖远和古浪L1黄土和SO古土壤具有相似的岩石磁学特征.磁性矿物含量相对较低,载磁矿物均以磁铁矿为主,同时含有磁赤铁矿和赤铁矿,且SO占土壤中的磁赤...     

Low temperature magnetic properties of basalts containing near ~TM30 titanomagnetite

The paper is devoted to studying the mineral composition and magnetic properties, mainly at the cryogenic temperatures, of the Middle–Late Devonian basalts from North Timan. The magnetic minerals in these basalts are dominated by intermediate-composition titanomagnetites (TM25–TM30) which demonstrate unusual magnetic properties in a wide temperature range. At room temperature, a low coercive force coexists with relatively high M_rs/M_s ratios. At cryogenic temperatures, the dependences of magnetic susceptibility on the temperature and frequency of the applied field are characteristic of this titanomagnetite composition, whereas the remanent saturation magnetization acquired at 2 K is destroyed at significantly lower temperatures compared to the synthetic analogs. The obtained results again highlight the necessity of studying the low-temperature properties of titanomagnetite samples with a controlled composition and grain size.     

密度非对称的二维无碰撞磁场重联

使用二维粒子模拟（PIC）的方法研究了在电流片两侧具有不同温度或密度情况下的无碰撞磁场重联过程.在初始等离子体密度非对称的情况下,发现重联区等离子体流场结构、电磁场结构以及重联过程与对称情况下的结果有明显不同.通过对电流片两侧温度比取不同的参数T_m/T_s=1,2,5进行模拟(其中T_m和T_s分别代表磁层侧和磁鞘侧的温度),结果分析发现,(1)在密度非对称系统中,出流区电子沿着分离面出现一个整体的从高密度区向低密度区的流动,并围绕磁岛形成一个电流环;(2)在高温低密度一侧,在重联过程中,分离面两侧将出现很强的电荷分离并产生一个基本垂直于分离面的强度较大的电场E_z,其幅度和空间尺度与温度梯度近似地成线性正比和反比关系.在初始电流片两侧温度之比取T_m/T_s=5的情况下,E_z的幅度将达到0.71,其空间尺度与局地电子惯性长度d_e同一量级,这一结果与观测相吻合;(3)重联率随着温度梯度增大而下降.     

The low-temperature electrical properties of carbonaceous meteorites

Electrical conductivities and dielectric constants have been measured over the temperature range 90–300°K on several carbonaceous chondrites and some terrestrial analogues. The conductivities of meteorites of different petrologic subtypes range over many orders of magnitude and the low-temperature activation energies are typically much smaller than those observed in terrestrial materials at higher temperatures. The electrical properties of carbonaceous chondrites vary systematically with chemical-mineralogical characteristics in that: (1) activation energy at low temperature is greater in the more volatile-rich meteorites containing hydrated silicates, and (2) conductivity is greater in the more reduced meteorites of higher petrologic subtype. These new data on the electrical properties of chondrites hold important implications for both the thermal and magnetic histories of small bodies in the early solar system.     

Magnetic reconnection as a possible heating mechanism of the local high temperature protons within magnetic clouds

Magnetic clouds have the outstanding observational features of low proton temperature and plasma beta value, but numerous observations show that some magnetic clouds often have local high temperature phenomena. The local high temperature protons may be heated by magnetic reconnections within magnetic clouds. Here we take the magnetic cloud on 18–20 October 1995 as an example to discuss the possible heating mechanism. There is a famous protuberance in proton temperature between the front boundary and 11: 00 UT on 19 October 1995. Eight magnetic reconnection events were identified within the magnetic cloud, whose duration was less than 31 hours, and most of these reconnection events occurred within the proton temperature enhanced part of the magnetic cloud. Hence, it is possible for the local protons in the magnetic cloud to be heated by magnetic reconnections.     

Rock magnetic criteria for the detection of biogenic magnetite

We report results on the magnetic properties of magnetites produced by magnetotactic and dissimilatory iron-reducing bacteria. Magnetotactic bacterial (MTB) strains MS1, MV1 and MV2 and dissimilatory iron-reducing bacterium strain GS-15, grown in pure cultures, were used in this study. Our results suggest that a combination of room temperature coercivity analysis and low temperature remanence measurements provides a characteristic magnetic signature for intact chains of single domain (SD) particles of magnetite from MTBs. The most useful magnetic property measurements include: (1) acquisition and demagnetization of isothermal remanent magnetization (IRM) using static, pulse and alternating fields; (2) acquisition of anhysteretic remanent magnetization (ARM); and (3) thermal dependence of low temperature (20 K) saturation IRM after cooling in zero field (ZFC) or in a 2.5 T field (FC) from 300 K. However, potentially the most diagnostic magnetic parameter for magnetosome chain identification in bulk sediment samples is related to the difference between low temperature zero-field and field cooled SIRMs on warming through the Verwey transition (T ≈ 100 K). Intact chains of unoxidized magnetite magnetosomes have ratios of δ_FC/δ_ZFC greater than 2, where the parameter δ is a measure of the amount of remanence lost by warming through the Verwey transition. Disruption of the chain structure or conversion of the magnetosomes to maghemite reduces the δ_FC/δ_ZFC ratio to around 1, similar to values observed for some inorganic magnetite, maghemite, greigite and GS-15 particles. Numerical simulations of δ_FC/δ_ZFC ratios for simple binary mixtures of magnetosome chains and inorganic magnetic fractions suggest that the δ_FC/δ_ZFC parameter can be a sensitive indicator of biogenic magnetite in the form of intact chains of magnetite magnetosomes and can be a useful magnetic technique for identifying them in whole-sediment samples. The strength of our approach lies in the comparative ease and rapidity with which magnetic measurements can be made, compared to techniques such as electron microscopy.     

Theoretical analysis of thermomagnetic properties, low-temperature hysteresis and domain structure of titanomagnetites

Magnetic hysteresis of coarse-grained titanomagnetites at room temperature is characterised by low coercive force, low relative remanence, and a high ratio of coercivity of remanence to coercive force. These properties are generally interpreted in terms of multidomain structure. At low temperatures, however, ulvöspinel-rich compositions exhibit hysteresis properties similar to those of single-domain assemblages, and on this basis Radhakrishnamurty and Deutsch have proposed an alternative interpretation of the domain structure of titanomagnetites having x 0.3 in terms of a mixture of single-domain and superparamagnetic particles. Low apparent Curie temperatures are attributed to the effects of thermal agitation above the blocking temperature.

We have examined theoretically the effects of thermal agitation on the low- and high-field thermomagnetic curves and find that observed Curie temperatures in general represent an intrinsic property of the magnetic mineral present, rather than reflecting thermal agitation. The high coercive force and relative remanence at low temperatures for titanomagnetites having x > 0.5 can be explained on the basis of the interaction of domain walls with crystal defects when the large increases in magnetocrystalline anisotropy and magnetostriction with decreasing temperature are taken into account. We discuss the evidence for the existence of domain walls in coarse-grained ulvöspinel-rich titanomagnetites and conclude that multidomain structure is well established.

It is also shown that fine titanomagnetite grains may have more than one blocking temperature. In any temperature interval for which superparamagnetic grains are present they will disproportionately influence susceptibility and low-field hysteresis.     

磁性矿物的磁学鉴别方法回顾

磁性矿物的组成和颗粒粒径的分布决定了岩石或沉积物的基本磁学性质及其所携带的天然剩磁在地质时期内的稳定性.由于自然界中磁性矿物的复杂性和多样性，如何有效的确定磁性矿物的成分和粒径分布一直是岩石磁学的基础和难点.本文对确定磁性矿物成分和粒径分布的常见方法进行了较为详细的总结和分析，并对常见磁性矿物在高温和低温下的磁学性质进行了详细的论述.最后对如何应用综合方法判定样品中的磁性矿物种类以及粒度分布进行了探讨.     

考古标本岩石磁性的初步研究

讨论了考古标本中所含矿物的磁学性质与古代地球磁场强度测定数据可靠性之间的关系,进行了岩石磁学实验,包括高温、低温磁化率测定、居里温度测定、磁滞回线各参数的测定等．结果表明,文中所用各类标本（陶片、砖、烧土等）的主要载磁矿物为磁铁矿,采用这些标本用Ｔｈｅｌｌｉｅｒ方法进行逐步热退磁实验所测定的古强度数据较为可靠．     

Some rock magnetic properties of mid-Cretaceous basalts from Israel and India (Rajmahal traps), and their bearing on palaeointensity experiments

A wide range of rock magnetic properties have been determined from two collections of mid-Cretaceous basalts; one from Israel, the other from the Rajmahal traps in northeast India. Deuteric oxidation is rare in both collections, with titanium-rich titanomagnetite being the principal remanence carrier in most cases. There are a number of differences in rock magnetic properties between the two groups. Some of these seem to be primary, whereas others appear to be caused by hydrothermal alteration and weathering, which are more prevalent in the Indian rocks. These rocks are being used in palaeointensity experiments, from which it is hoped to determine the strength of the Earth's magnetic field during the long period of normal polarity in the mid-Cretaceous. Thellier palaeointensity experiments have been performed on two samples from each site. The degree of agreement between the two results is highly variable. The low blocking temperatures and the presence of secondary viscous components in many samples make Thellier palaeointensity experiments very difficult. A further problem is that of thermal alteration, two main types of which are observed. The first manifests itself as a large and sudden increase in partial thermoremanent magnetization (pTRM) capacity, and the second as a steady decrease in the size of pTRM with increasing temperature.     

地热地球物理勘探新进展

地热作为一种清洁能源具有巨大的开发潜力,将在我国的经济发展中起到巨大的作用.在传统的热水型地热开发的基础上,国际上非常重视热干岩(Enhanced Geothermal)型地热的勘探开发.在这两类地热勘查和开发中,地球物理方法具有非常重要的作用.本文从地热系统的目标体岩石的地球物理性质出发,分析岩石的地球物理性质与温度、压力和含水量等影响因素的关系.例如随着温度的升高,岩石会出现去磁、电阻率降低、密度降低、弹性波速度也现明显降低等现象.进而分析地球物理方法应用到具体的地热勘查地质-地球物理异常模型.结合国际上21世纪以后的新方法技术,分析了重磁、电、地震方法在利用由于岩石温度的升高而出现的特殊地球物理现象,并应用于地热勘探.通过国内外实例介绍了各种地球物理勘探方法在地热勘查中成功应用,为进一步提高我国地热勘查水平,提供一些参考.