Solar radio burst (type III)     

Hari Om Vats  M. R. Deshpande  K. N. Iyer  Tetsuro Kondo  Takeshi Isobe 《Astrophysics and Space Science》1996,243(1):251-254

This article describes the observations of a type III radio burst observed at 103 MHz simultaneously by the two radio telescopes situated at Rajkot (22.3°N, 70.7°E) and Thaltej (23°N, 72.4°E). This event occurred on September 30, 1993 at about 0430 UT and lasted for only half a minute. The event consisted of several sharp spikes in a group. The rise and fall time of these are comparable, however the peaks of individual spikes varied by a factor of four. The comparison of these observations with the data of solar radio spectrograph HiRAS indicates that this was a metric radio burst giving highest emission at about 103 MHz.  相似文献   

太阳活动高峰年山东区域电离层时空变化研究   总被引：1，自引：1，他引：0  

史坤朋  郭金运  董正华  周长志 《测绘科学》2017,(12):32-38

2012年为太阳活动高峰年份,为了研究太阳活动高年区域电离层的变化特征,该文选取了山东区域内的SDCORS站点,构建了山东区域垂直电子含量(VTEC)球谐格网模型,对该年山东区域电离层时空变化规律进行分析。实验研究表明,在空间变化上山东区域电离层表现出较强的纬度相关性,出现了明显的分层现象。同时给出了山东电离层在时间上呈现出的时段变化、日变化、月变化、季节变化,发现VTEC受太阳活动影响较大,除了存在明显的单峰和双峰结构外,该年还发生了半年度异常现象。  相似文献   

不同NeQuick电离层模型参数的应用精度分析   总被引：3，自引：2，他引：1  

王宁波  袁运斌  李子申  李敏  霍星亮 《测绘学报》2017,46(4):421-429

Galileo采用NeQuick作为全球广播电离层模型,其实际应用中以有效电离水平因子Az代替太阳活动指数作为NeQuick的输入参数,并利用二次多项式拟合得到广播星历中播发的3个电离层参数。本文在总结和讨论NeQuick模型参数估计方法及其变化特征的基础上,分别以全球电离层格网、GPS基准站及JASON-2测高卫星提供的电离层TEC为参考,分析不同NeQuick模型参数(包括以太阳活动参数F10.7为输入的NeQuick2、以本文解算参数为输入的NeQuickC和以Galileo广播电离层参数为输入的NeQuickG)在全球大陆及海洋地区的应用精度,并与GPS广播的Klobuchar模型对比。结果表明,NeQuickG在全球范围内的修正精度为54.2%~65.8%,NeQuickC的修正精度为71.1%~74.2%,NeQuick2的修正精度与NeQuickG相当,略优于GPS广播星历中播发的Klobuchar模型。  相似文献   

山西保德—静乐地区新近纪地层时代讨论     

朱大岗  孟宪刚  邵兆刚  雷伟志  王津  韩建恩  余佳  吕荣平  王艳 《地质通报》2008,27(4):510-516

通过对山西保德-静乐地区新近纪地层的野外地质调查和实测剖面,对分布于该区的新近纪地层进行了详细的研究和划分,获得了新的ESR和古地磁测年数据,并结合生物地层序列确定了该区新近系地层的顺序为：新近系上新统静乐组（N2j）、新近系中新统上部保德组（N1^26）和中新统下部芦子沟组（N1^1l）。  相似文献   

电离层电子浓度总含量梯度对GPS差分定位精度的影响     

徐于月  黄张裕  陈苏娟 《测绘工程》2008,17(2):30-33

针对GPS定位测量的信号传播路径误差,分析了电离层电子浓度总含量梯度对差分定位精度的影响,利用L1载波重点讨论了1999年-2000年太阳活动期间低纬度赤道异常地区GPS差分定位精度的问题,同时验证对于长基线采用GPS广域差分技术可以使电离层定位误差得到明显提高。  相似文献   

Identification of Uranyl Minerals Using Oxygen K‐Edge X‐Ray Absorption Spectroscopy          下载免费PDF全文

Jesse D. Ward  Mark Bowden  C. Tom Resch  Steven Smith  Bruce K. McNamara  Edgar C. Buck  Gregory C. Eiden  Andrew M. Duffin 《Geostandards and Geoanalytical Research》2016,40(1):135-148

Although most of the world's uranium exists as pitchblende or uraninite, this mineral can be weathered to a great variety of secondary uranium minerals, most containing the uranyl cation. Anthropogenic uranium compounds can also react in the environment, leading to spatial–chemical alterations that could be useful for nuclear forensics analyses. Soft X‐ray absorption spectroscopy (XAS) has the advantages of being non‐destructive, element‐specific and sensitive to electronic and physical structure. The soft X‐ray probe can also be focused to a spot size on the order of tens of nanometres, providing chemical information with high spatial resolution. However, before XAS can be applied at high spatial resolution, it is necessary to find spectroscopic signatures for a variety of uranium compounds in the soft X‐ray spectral region. To that end, we collected the near edge X‐ray absorption fine structure (NEXAFS) spectra of a variety of common uranyl‐bearing minerals, including uranyl carbonates, oxyhydroxides, phosphates and silicates. We find that uranyl compounds can be distinguished by class (carbonate, oxyhydroxide, phosphate or silicate) based on their oxygen K‐edge absorption spectra. This work establishes a database of reference spectra for future spatially resolved analyses. We proceed to show scanning X‐ray transmission microscopy (STXM) data from a schoepite particle in the presence of an unknown contaminant.  相似文献   

新疆北山小常山铁矿矿物电子探针分析及矿床成因探讨          下载免费PDF全文

张博  吕新彪  刘月高 《岩石矿物学杂志》2016,35(3):517-530

小常山铁矿位于新疆北山裂谷带西段,矿体赋存于辉长岩、辉长岩和大理岩接触带中,部分赋存于花岗闪长岩和大理岩接触带。前人研究辉长岩年龄为276±1.2Ma,与坡北铜镍硫化物岩浆矿床形成年龄一致,同属早二叠世。小常山铁矿中可见有明显的岩浆贯入现象。矿体主要呈透镜状、块状、脉状、薄层状。金属矿物主要为磁铁矿,含极少量的褐铁矿和黄铁矿;近矿围岩蚀变较弱,主要有石榴子石化、绿帘石化、大理岩化。电子探针研究表明,磁铁矿FeOT含量范围较大,主要分布在85%范围以上,Al_2O_3含量相对较高,TiO_2-Al_2O_3-(MgO+MnO)图解、TiO_2-Al_2O_3-MgO图解均显示热液接触交代成因特点,表明小常山铁矿的形成和岩浆热液的交代作用有关。石榴子石属于钙铝榴石-钙铁榴石系列,与典型矽卡岩矿床的石榴子石端员组分组成有一定差别。结合小常山铁矿体地质特征以及电子探针分析测试等研究,认为小常山铁矿是多成因的复合型矿床,具有岩浆成因和热液成因特征,但后者是主要成因。  相似文献   

Microstructural characteristics of the Whitby Mudstone Formation (UK)     

《Marine and Petroleum Geology》2016

When trying to improve gas productivity from unconventional sources a first aim is to understand gas storage and gas flow potential through the rock by investigating the microstructure, mineralogy and matrix porosity of unfractured shale. The porosity and mineralogy of the Mulgrave Shale member of the Whitby Mudstone Formation (UK) were characterized using a combination of microscopy, X-ray diffraction and gas adsorption methods on samples collected from outcrops. The Whitby Mudstone is an analogue for the Dutch Posidonia Shale which is a possible unconventional source for gas. The Mulgrave shale member of the Whitby Mudstone Formation can microstructurally be subdivided into a fossil rich (>15%) upper half and a sub-mm mineralogically laminated lower half. All clasts are embedded within a fine-grained matrix (all grains < 2 μm) implying that any possible flow of gas will depend on the porosity and the pore network present within this matrix. The visible SEM porosity (pore diameter > 100 nm) is in the order of 0.5–2.5% and shows a non-connected pore network in 2D. Gas adsorption (N2, Ar, He) porosity (pore diameters down to 2 nm) has been measured to be 0.3–7%. Overall more than 40% of the visible porosity is present within the matrix. Comparing the Whitby Mudstone Formation to other (producing) gas shales shows that the rock plots in the low porosity and high clay mineral content range, which could imply that Whitby Mudstone shales could be less favourable to mechanical fracturing than other gas shales. Estimated permeability indicates values in the micro-to nano-darcy range.  相似文献   

无内标-多外标校正激光剥蚀等离子体质谱法测定磁铁矿微量元素组成   总被引：4，自引：2，他引：2  

孟郁苗  黄小文  高剑峰  戴智慧  漆亮 《岩矿测试》2016,35(6):585-594

激光剥蚀电感耦合等离子体质谱(LA-ICP-MS)常用于磁铁矿原位微量元素分析,按照校正策略不同,主要分为内标法和无内标法。内标法需要用电子探针(EMPA)预先测定磁铁矿中内标元素Fe的含量,过程较繁琐,且待测元素含量会受到内标元素含量测定的影响。本文采用铁含量较高的玄武质玻璃BCR-2G、BIR-1G、BHVO-2G和GSE-1G作为外标,避免了内标元素含量的测定,建立了无内标-多外标校正LA-ICP-MS测定磁铁矿微量元素组成的分析方法。利用该方法测定了科马提岩玻璃GOR-128g和自然岩浆磁铁矿BC 28的微量元素组成以评估方法的可靠性。结果表明,科马提岩玻璃的测定结果与推荐值及前人内标法的测定值一致,多数元素的相对标准偏差RSD5%;自然岩浆磁铁矿的测定结果与推荐值相比,多数元素的RSD7%,低于前人内标法的RSD(15%)。由此说明无内标-多外标法可以实现富铁硅酸岩或磁铁矿微量元素含量的准确校正,克服了基体效应的影响。因此,无内标-多外标法是一种原位测定磁铁矿微量元素含量的快速、准确方法,具有一定的应用潜力。  相似文献   

含AgI焰剂成冰性能与物化特征的实验研究     

孔君  王广河  房文  苏正军 《气象》2016,42(1):74-79

利用CAMS的1 m~3等温云室系统筛选出新型高效AgI焰剂WMC-IN-001和WMG-IN-002。检测结果表明,它们具有较高的成核率,在-15℃时达到10~(15)g~(-1)AgI量级,尤其在-7℃时WMC-IN-001的成核率仍可达到10~(14)g~(-1)AgI量级。同时给出对节银剂配方和2011年市场上主要的几种催化剂的检测结果进行对比。WMC-IN-001和WMC-IN-002的成冰速率较慢,在各检测温度的成冰速率差异较小,均在40~55 min。利用冷场发射扫描电镜和能谱仪对WMC-IN-001燃烧产生的气溶胶粒子作了物化特征分析,粒子分布在0.02~0.60μm,具有两个典型的模态:0.02~0.10μm的较小的粒子和0.20~0.55μm的较大的粒子,均立方直径为0.2472μm。WMC-IN-001气溶胶粒子明显偏大,小粒子相对较少,这可能是其成冰速率偏慢的原因之一。  相似文献