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1.
基于漫反射光谱(DRS)的铁氧化物定量分析已用于北方黄土的研究,而在南方黄土中的适用性尚不清楚。本文选取江西九江黄土为研究对象,采用柠檬酸钠-重碳酸钠-连二亚硫酸钠(CBD)方法去除其中的游离铁,以此为基体分别加入不同比例的赤铁矿和针铁矿,通过多元线性回归方法建立了标样的铁氧化物含量与光谱反射率之间的校准方程。经检验,校准方程应用于未经CBD处理的剖面天然样品时,获得的赤铁矿含量较准,而针铁矿含量不准。原因可能在于:(1)混合体系中,赤铁矿与针铁矿互为基体,赤铁矿对针铁矿的干扰远大于针铁矿对赤铁矿的影响,这种差异在南方地区尤为明显;(2)CBD处理不能完全清除南方黄土中的针铁矿,可能与样品中含有部分结晶较好、粒度较粗的针铁矿有关,这也增加了针铁矿定量分析的不准确性;(3)铝的同晶替代现象对南方黄土影响更为显著,其中受晶格结构等影响,针铁矿的铝替代量比赤铁矿更大,可能对定量分析结果的准确性影响也更大。因而在南方黄土中,基于DRS的铁氧化物定量分析方法对于赤铁矿是适用和有效的,对于针铁矿的应用则需要慎重。 相似文献
2.
长江三角洲东延海域嵊山岛屿风尘堆积地层是记录晚更新世晚期东亚季风演变的重要载体。采用漫反射光谱（DRS）法、柠檬酸钠-重碳酸钠-连二亚硫酸钠（CBD）浸提法结合标准赤铁矿、针铁矿建立标准铁氧化物含量与反射率之间的校准方程，定量重建了东部岛屿风尘堆积的赤铁矿、针铁矿含量的变化特征。结果显示，东海嵊山岛风尘堆积中赤铁矿的含量为0.18%~0.40%，平均值为0.31%，针铁矿的含量为0.7%~1.19%，平均值为1.11%。根据赤铁矿、针铁矿含量特征结合地球化学和环境磁学参数，分析其记录的古环境信息:54~46 ka B.P.时期内气候相对干燥，季风降水减弱，46~39 ka B.P.时期内气候相对潮湿，季风降水增强；46±4 ka B.P.时期的高值可能指示了一个冷事件。 相似文献
3.
运用岩石磁学和地球化学相结合的方法对宝鸡剖面S5和S3古土壤的磁性特征进行了详细对比分析,结果表明S5古土壤层Rb/Sr比值较高,S5古土壤形成期气候温暖湿润,成壤程度比S3时期强.S5层亚铁磁性矿物含量低于S3层,反铁磁性矿物主要为针铁矿;而S3层的反铁磁性矿物主要为赤铁矿.S5层土体表面及土壤空隙中可见大量黑褐色的铁锰胶膜分布,由于沉积后土壤长时期处于偏干或偏湿的氧化、还原交替环境中,细粒的磁铁矿和/或磁赤铁矿、赤铁矿溶解转化成褐铁矿、针铁矿等弱磁性矿物,主要转化成在局域湿润环境下能够稳定存在的针铁矿,这种磁性矿物的转化可能导致了成壤强的S5古土壤超顺磁亚铁磁性矿物含量的减少和磁化率的降低. 相似文献
4.
川西高原河谷阶地和断陷盆地广泛分布厚层风成黄土-古土壤序列,目前对其磁学性质变化机制及古气候意义研究还很薄弱。文章对该区理县黄土-古土壤剖面进行了系统的岩石磁学研究,确定了其磁性矿物种类、含量和颗粒大小的特征及其变化规律。通过结合粒度、色度与地球化学参数,进一步探讨了理县黄土-古土壤磁性的主控因素。结果表明:1)理县剖面同时含有强磁性矿物(为磁铁矿和磁赤铁矿)以及弱磁性矿物(为赤铁矿和针铁矿);2)相对黄土层,古土壤层含有更高比例的亚铁磁性矿物;3)成土过程中生成的大量细小强磁性矿物颗粒,是古土壤层S1磁化率增加的主导因素,该模式与黄土高原相似;4)结合色度以及磁学性质,可以较为明确地区分成壤强度;(5)理县黄土剖面物源复杂,磁学特征受到沉积物来源、后期流水和气候的共同作用,利用单一磁学性质(比如磁化率)进行古气候研究会造成多解性。 相似文献
5.
新疆尼勒克黄土岩石磁学特征及变化机制研究 总被引：1，自引：0，他引：1
新疆黄土与黄土高原黄土相比,无论在物源还是后期成土环境方面都存在较大差异,因此二者的磁学特征有所不同。本文选取伊犁尼勒克地区的一个黄土-古土壤剖面进行了系统的岩石磁学及粒度研究。实验结果表明尼勒克剖面中磁性矿物具有以下特征:1)以亚铁磁性矿物磁铁矿和磁赤铁矿为主,并含有一定量的反铁磁性矿物赤铁矿和针铁矿;2)各黄土层成壤作用弱,磁性矿物以原始输入的粗颗粒MD和PSD为主。PS_1古土壤层成壤作用强,以细颗粒SD为主。弱发育古土壤层PS。既包含SD颗粒,又有粗颗粒。各地层均不含SP颗粒;3)PS_1古土壤层原始含铁矿物输入量略低于黄土高原地区,其他各地层均高于黄土高原地区,但受成土作用及其他因素影响,剖面中亚铁磁性矿物含量远低于黄土高原黄土-古土壤层。PS_1古土壤层成壤作用强,在新疆地区较为少见,但其磁化率却低于各黄土层,说明尼勒克黄土-古土壤磁化率变化机制与黄土高原地区不同。古土壤层原始输入含铁矿物的量较黄土层低,但原始含铁矿物只是影响剖面磁化率变化的原因之一。PS_1古土壤层在沉积后期受到间歇性水流作用,成土成因的强磁性SP磁铁矿/磁赤铁矿颗粒遭受破坏并转化为赤铁矿,导致PS_1古土壤层磁化率的急剧降低,并使该层赤铁矿的相对含量增加。 相似文献
6.
罗马尼亚第四纪黄土沉积的岩石磁学特征及成土模式探讨 总被引：1，自引：0，他引：1
欧洲罗马尼亚发育着典型的第四纪风积黄土-古土壤地层,通过对Mircea Voda剖面黄土-古土壤样品进行磁化率、频率磁化率、非磁滞剩余磁化强度、等温剩磁、热磁曲线和磁滞回线等岩石磁学参数测试分析,发现罗马尼亚Mircea Voda黄土-古土壤序列磁化率曲线形态与中国黄土高原中部西峰黄土极为相似;而且所含磁性矿物种类也很相似,主要以亚铁磁性矿物(磁铁矿和磁赤铁矿)为主,也含有反铁磁性矿物(赤铁矿和针铁矿).罗马尼亚Mircea Voda黄土与中国西峰黄土有相似的成土模式,成土过程都是在干旱氧化环境中进行,磁化率与成土作用基本成正相关关系.磁化率在成土弱的黄土层中获低值,在成土强的古土壤层中获高值,反映冰期、间冰期旋回在全球范围内对气候影响的一致性.成±过程粒度小的超顺磁(SP)和单畴(SD)亚铁磁性矿物相对含量的增加是罗马尼亚Mircea Voda剖面古土壤磁化率增强的主要原因.罗马尼亚Mircea Voda黄土的磁化率数值整体低于中国西峰黄土的值,物源的差异以及罗马尼亚气候的水热不同期使得古土壤发育弱于中国黄土,以及地下水对剖面底部土壤层的淋溶作用,可能是造成Mircea Voda黄土磁化率低于西峰黄土的原因. 相似文献
7.
赤铁矿和针铁矿是自然界中最稳定的两种铁氧化物,广泛存在于地球的各个圈层。很多沉积物的颜色都是由它们引
起的,它们的形成和保存具有重要的环境指示意义。实验室中赤铁矿和针铁矿的表征和鉴定手段很多,但受其含量低、结
晶差、颗粒细小难分离等因素的困扰以及某些测试方法自身的限制,能用于铁氧化物定量分析的方法很少。文中就常用的
基于X射线衍射（XRD） 和漫反射光谱（DRS） 的铁氧化物定量方法进行了系统评价。在定性分析的基础上,采用基于
XRD的K值法获得西藏床得剖面红色页岩中赤铁矿的含量为3.81％~8.11％,采用DRS与多元线性回归相结合的方法获得北
大西洋ODP1049C孔12X岩芯段棕色层中赤铁矿和针铁矿的含量分别为0.13％~0.82％和0.22%~0.81％,橙色层中赤铁矿和
针铁矿的含量分别为0.19%~0.46％和0.29%~0.67％。与其它分析结果的比较表明,这两种定量方法在白垩纪大洋红层中的
应用是可行的。但在实际应用时,首先要通过XRD和DRS相结合来提高定性分析的准确性,然后通过综合分析铁氧化物的
预判含量范围和结晶程度来选择合适的定量方法。 相似文献
8.
从西峰和段家坡黄土剖面S5-1层段中分选出<30μm粒级、磁性相对最强的组分(分别为XS-4J和DS-4J),先后进行了MPV-3光学显微镜的观察与反射率测定、矿物的扫描电镜能谱测定和X射线衍射物相分析.两个样品的磁性矿物均以风尘碎屑状的钛铁氧化物为主.XS-4J样矿物的反射率和Fe的含量都普遍较高,磁性矿物除磁(赤)铁矿、赤铁矿外还见有含铁高的氧化物(Fe 72.20%～86.70%,质量分数)和含Cr、Ni的钛铁晶石或钛铁矿.DS-4J样的磁性矿物中Fe与Ti元素呈明显的负线性相关关系,Si、Al、Ca的含量较高,矿物以磁(赤)铁矿、赤铁矿、针铁矿和褐铁矿为主,并明显见有磁性矿物被溶蚀和新生的磁(赤)铁矿.磁性矿物成分与组合特征的差异反映了西峰与段家坡S5-1岩石中磁性矿物的物质来源与保存条件有较明显的差异. 相似文献
9.
沉积物-古土壤是记录古环境演化及古气候变迁的有效载体,利用沉积物-古土壤对气候环境信息的记录来研究全球变化问题,已成为当前地球科学研究的热点课题。赤铁矿和针铁矿是沉积物-古土壤中常见的次生矿物,二者含量的变化能有效反映成土过程中冷、暖、干、湿的变化。然而,赤铁矿和针铁矿在沉积物-古土壤中结晶度差且含量低,因此,对二者进行有效定量一直是研究的难题。近年来,漫反射光谱(DRS)分析在沉积物-古土壤中赤铁矿和针铁矿的定量研究中取得了一系列显著的成果。本文系统总结了漫反射光谱在赤铁矿和针铁矿定量中的原理,并对3种常见定量方法及其应用进行归纳,同时对定量过程中存在的问题和发展趋势进行深入讨论。 相似文献
10.
新疆黄土岩石磁学特征与地层性质的对应关系具有鲜明的区域特征.本文选取沙湾黄土剖面进行较为系统的岩石磁学分析.研究结果表明,沙湾剖面的磁性矿物组成与黄土高原及新疆北部其他黄土剖面相似,以亚铁磁性矿物(如磁铁矿、磁赤铁矿)为主要的载磁矿物,同时含有一定量的不完全反铁磁性矿物(如赤铁矿、针铁矿)和顺磁性矿物.假单畴(PSD)和多畴(MD)为样品的主要磁畴特征,部分土壤样品中磁性矿物磁畴状态表现为单畴(SD).进一步分析发现,磁化率与地层对应关系较为复杂,剖面3m以上地层中的磁化率及其他相关磁学参数与成壤强度呈现正相关关系,全新世以来发育的古土壤中磁化率值较高,细颗粒磁性矿物含量也较高;而3m之下地层中磁学参数显著表现为风力强度驱动变化模式.古风场强度的变化可能对剖面整体磁学性质具有一定的影响,成壤作用受到风动力条件的制约,主要决定了较细颗粒磁性矿物的含量变化.xARM/SIRM参数与磁化率相比对地层成壤强度的指示作用更为明显. 相似文献
11.
Weiguo Zhang Lizhong Yu Min Lu Xiangmin Zheng Junfeng Ji Limin Zhou Xiaoyong Wang 《Quaternary Science Reviews》2009,28(3-4):345-353
The Xiashu Loess, in comparison to the well-studied loess sequences in the Chinese Loess Plateau (CLP), provides a good opportunity for studying East Asian monsoon variations from a southern China perspective. Here we present a study of the iron oxide mineralogy of the Xiashu Loess using integrated geochemical and diffuse reflectance spectroscopy (DRS) measurements as well as magnetic data. Our results show that the free iron oxide (Fed) to total iron (Fet) ratio (Fed/Fet), hematite (Hm) to goethite (Gt) ratio (Hm/Gt) and saturation isothermal remanent magnetization (SIRM) to magnetic susceptibility (χ) ratio (SIRM/χ) all indicate particularly strong summer monsoons during the formation of paleosols PS5 and PS4 (equivalent to Marine Isotope Stage 13 and 11, respectively). However, magnetic susceptibility and Fed/Fet are not consistently reliable indicators of summer monsoon intensity for the whole section. Our results indicate that a multi-proxy approach can give a more reliable summer monsoon intensity reconstruction. The summer monsoon shows a cooling trend and a declining of precipitation from 0.5 to ～0.3 Ma, after which it becomes warmer and wetter towards the top of paleosol PS1 (equivalent to MIS 5). However, PS1 was formed under a relatively cooler temperature and wetter soil conditions in comparison to PS5 and PS4. Such supra-orbital variations in the East Asian summer monsoon superimposed on the effects of glacial–interglacial cycles in southern China are also reflected in the 0.4–0.5 Ma cycle of marine carbon isotopes in the global ocean, possibly indicating a strong link between terrestrial weathering and the global carbon cycle. 相似文献
12.
On the basis of a key model of the appearance of hematite and goethite in some Chinese and European loess successions, paleosols generally contain higher proportions of hematite formed by pedogenic processes during warm and humid interglacials, while loess contains sedimentary goethite deposited during colder, glacial periods. Rock magnetic measurements were conducted on samples from Paks (Hungary) loess, revealing an anomalous case. Sediments were found to contain higher amounts of hematite and/or goethite, while the well‐developed paleosols were found to be lacking in hematite but had significant amounts of magnetite and maghemite. This observation demonstrates that the character of pedogenic magnetic mineral alteration and neoformation differs from the hematite/goethite model; the model is therefore not applicable to the Paks succession, possibly due to differences in the regional paleoclimate and pedogenic environment. The results indicate the existence of a further model, in which hematite formation is not significant in the course of pedogenesis. 相似文献
13.
Zr/Rb ratio in the Chinese loess sequences and its implication for changes in the East Asian winter monsoon strength 总被引：2，自引：0，他引：2
The long-term dust accumulation sequences on the Chinese Loess Plateau (CLP) provide a valuable opportunity to study the evolution of East Asian winter monsoon strength. Grain size of bulk samples of loess deposits, though widely used, is a modified measure of the strength of winter monsoon wind due to modification by post-depositional weathering and pedogenesis. This study proposes a new and reliable geochemical climate proxy that records the variability of the East Asian winter monsoon on the CLP. Six loess-paleosol sections on the Plateau were selected for measuring concentrations of the trace elements Zr and Rb as well as grain size. Variations of the Zr/Rb ratio in all the sections encompassing the last 130 ka display a generally similar pattern to that of mean grain size of bulk samples (MGSB). Though a positive correlation exists between the Zr/Rb ratio and MGSB, the correlation coefficient decreases in southern and eastern sections where intense pedogenesis occurred in the relatively warm and humid climates. Long-term Zr/Rb variation in the Lingtai section exhibits amplitudes and frequencies similar to those in MGSB and the mean grain size of quartz particles (MGSQ, accepted as a more reliable proxy than MGSB) in the upper loess-paleosol sequence over the past 2.6 Ma. However, for the underlying Red Clay formation, in the interval from about 7-2.6 Ma B.P., the MGSB record is relatively stable, whereas both the Zr/Rb ratio and MGSQ show distinct variability and display amplitudes similar to those observed in the overlying loess-paleosol sequence. These results demonstrate that the Zr/Rb ratio reflects original eolian grain size and may serve as a reliable index of the strength of East Asian winter monsoon winds. 相似文献
14.
东秦岭地区黄土堆积的岩石磁学特征及磁化率增强机制探索 总被引：2，自引：0，他引：2
对东秦岭地区洛南盆地的上白川、刘湾和丹江上游的二龙山黄土剖面进行了岩石磁学研究。结果表明,大部分黄土和古土壤样品的磁性矿物以磁铁矿和磁赤铁矿为主,古土壤中亚铁磁性矿物的含量比黄土的多,极少数黄土样品以反铁磁性矿物为主。亚铁磁性矿物和反铁磁性矿物的含量随成土作用增强而增加,成土作用形成的细粒亚铁磁性矿物包括超顺磁性和单畴（似单畴）颗粒,但以单畴和（或）似单畴为主。古土壤磁化率增强与这些土壤成因的细粒亚铁磁性矿物含量有关,显示出受气候变化控制的特点。东秦岭地区黄土岩石磁学性质与黄土高原地区的相似,但也存在一定差异,而且三个剖面之间磁化率值整体差别较大。温湿的气候和复杂的山区地形可能是导致这种差异的原因。 相似文献
15.
陕南丹凤茶房村黄土-古土壤剖面色度参数特征 总被引：2，自引：1，他引：1
以丹凤县茶房村黄土-古土壤剖面为对象, 研究了该区黄土色度参数的变化规律及其主控因素。结果表明, L*(亮度)在黄土层中出现峰值, a*(红度)、a*/b*(红度/黄度)在古土壤层出现峰值, 色度参数的峰谷变化特征与该区黄土-古土壤地层旋回相吻合。L*(亮度)的变化与有机质含量密切相关;a*(红度)、a*/b*(红度/黄度)的变化则受控于铁氧化物的种类和含量。尽管三者的受控因素不同, 但都与风化成壤强度密切相关, 且与磁化率形成良好的对比, 可作为良好的气候代用指标, 间接地反映该区气候和成壤环境的变化规律。 相似文献
16.
Mineral forms of iron oxide, such as hematite, goethite and jarosite, are important because they are widely distributed at the Earth’s surface and because they are used as indicators for mineral exploration. Iron oxide abundance in rocks containing these minerals can be estimated from the absorption depth at wavelengths of around 900 nm in a reflectance spectrum, but this depth is also affected by extraneous factors such as grain size and topography. This paper investigated the effect of grain size on reflectance spectra and proposed a method for estimating iron oxide abundance in surface rocks by using remotely sensed data with suppression of the effects of grain size and topography. Reflectance spectra were measured in a laboratory from rock powder samples of different grain sizes containing iron oxide minerals. While the reflectance increased with decreasing grain size, the presence of ferric iron caused the absorption depth to be almost constant at around 900 nm, irrespective of the chemical composition of the sample. In addition, the difference between the reflectance at 550 nm and 760 nm (Slope) was a function of grain size. Iron oxide abundance can be estimated accurately by MCR-900D, which is the maximum absorption depth at the absorption center after the effect of grain size and topography was suppressed by Slope and the continuum-removal method, which takes the ratio between the original spectrum and its continuum, respectively. Correlation of MCR-900D results with datasets of actual spectral and chemical iron oxide laboratory measurements revealed that the mineral forms also need to be considered. MCR-900D results were significantly correlated with rock samples classified as containing different forms of iron oxide minerals (hematite, goethite and jarosite). Finally, MCR-900D was applied to an AVIRIS dataset for the Cuprite site in Nevada, USA. The results represented the enrichment zones of iron oxide within hydrothermally altered areas. 相似文献
17.
New insight into the structure of nanocrystalline ferrihydrite: EXAFS evidence for tetrahedrally coordinated iron(III) 总被引：1，自引：0，他引：1
Fabien Maillot Yuheng Wang Philippe Ildefonse Corinne Chaneac 《Geochimica et cosmochimica acta》2011,75(10):2708-9890
Ferrihydrite (Fh) is a short-range ordered nanocrystalline iron(III) (oxyhydr)oxide that has been recognized to play an important role in contaminant sequestration and in iron cycling in geological and biological systems. Despite intensive research for the two last decades, the structure of Fh is still a subject of debate. In the present study, we report extended X-ray absorption fine structure (EXAFS) spectroscopy data collected on a large set of ferrihydrites and model compounds samples including especially nano-crystalline maghemite (Mh), goethite (Gt), and akaganeite (Aka). This set of EXAFS data recorded at cryogenic temperature over a wide energy range allows us to precisely determine the Fe-O mean distance (〈Fe-O〉) in the first coordination shell of iron for this large set of iron (oxyhydr)oxides. Our EXAFS analysis includes both classical shell-by-shell fits of Fourier-filtered and unfiltered data as well as analysis of Fe-O distance distribution in the first coordination shell of iron using the Landweber iteration method. 〈Fe-O〉 determined by these complementary EXAFS analyses are similar: 〈Fe-O〉 is shorter in Mh (1.96 ± 0.01 Å) that contains 37.5% of tetrahedral iron, than in Gt (2.01 ± 0.01 Å), Aka (2.00 ± 0.01 Å) and hematite (Hm) (2.01 ± 0.01 Å) that do not contain tetrahedral iron. 〈Fe-O〉 for the five Fh samples investigated (1.97 ± 0.01 Å) was found to be slightly longer than in Mh and significantly shorter than those in Gt, Aka and Hm. This short 〈Fe-O〉 distance in Fh indicates the presence of significant amount of tetrahedrally coordinated iron(III) in all Fh samples studied, which ranges between 20 ± 5% and 30 ± 5% of total iron. In addition, our analysis of Fe-Fe distances observed by EXAFS is consistent with a Keggin-like motif at a local scale (∼5 Å) in the Fh structure. 相似文献
18.
最近13万年来黄土高原黄土剖面中绿泥石的化学风化与古气候变迁 总被引：4，自引：0，他引：4
对黄土高原不同纬度地区的4个黄土—古土壤剖面和lO个现代土壤样品中绿泥石的化学风化进行研究，发现黄土—古土壤剖面中的绿泥石在最近13万年发生了明显的化学风化，其风化程度受剖面位置和气候控制；黄土—古土壤剖面中ω(绿泥石 高岭石)／ω(伊利石)的比值与磁化率之间具有良好的负相关关系，绿泥石的化学风化与古土壤中铁氧化物矿物的形成和磁化率的增强之间有成因联系；黄土高原现代地表样品中ω(绿泥石 高岭石)／ω(伊利石)比值与现代年平均温度和年平均降水量有着良好的相关关系。认为ω(绿泥石 高岭石)／ω(伊利石)的比值可作为新的指示夏季风变化的替代性指标，对于定量重建古气候的变迁历史具有重要意义。 相似文献
19.
Magneticmineralsintheloess paleosolseriesaccountforabout 1 % -2 %ofthetotal (LiuTungshengandZhangZhonghu ,1 962 ) .Duetotheiraerolianorigin ,themagneticmineralsarecomplicatedincomposition ,largeingrainsizerange ,andsignificantlydifferentincrystallinity .Asaresult,researchonthesemagneticmineralswouldbesetwithalotofdifficulties.Previousre searchersemployedopticalmicroscopic ,X raydiffractionandM ssbauerspectrometrictechniquestostudythemagneticmineralsintheloess paleosolseries,andchieflyontheb… 相似文献