内蒙白云鄂博矿区H9中火山岩岩石特征及其意义

白云鄂博矿区Ｈ＿９地层岩石被中外学者长期看作是板岩或页岩，经近期研究发现岩性极为复杂。Ｈ＿９地层岩石是一套呈互层产出的粗面岩、流纹岩、流纹英安岩、变辉绿岩、白云岩、石英岩、黑云母岩、钠闪石－长石岩、钠辉石－长石岩、红柱石－黑云母角岩及碳质绢云板岩等。文中详细论述了这些火山岩石的结构构造、矿物成分和岩石化学成分，以及微量元素。对Ｈ＿９地层中火山岩，尤其是粗面质火山碎屑岩的确定，对了解白云鄂博矿床的成因和白云鄂博群形成的地质背景有重要意义。     

沉井下沉阻力离心模型试验研究

如何正确计算沉井的下沉阻力一直是沉井结构设计的难点,为了更加深入地研究沉井下沉阻力及其分布规律,通过离心机模型试验分别对4组不同埋深工况下的沉井进行了下沉模拟,对沉井侧壁土压力、刃脚斜面土压力、刃脚踏面土压力、沉井内外土面沉降进行了分析。研究结果表明：侧壁土压力随入土深度的增加呈先增大后减小的趋势,可采用分段函数形式对其大小及分布形式进行简化计算;刃脚斜面土压力呈三次多项式分布形式;随着刃脚入土深度的增加,刃脚斜面与踏面土阻力均显著增大,而单位投影宽度刃脚斜面与踏面土阻力比基本保持不变;沉井下沉会导致井外土面沉降,井内紧靠沉井内壁的土面沉降,离沉井内壁有一定距离的土面隆起。上述试验与分析成果可为理论研究与工程设计提供参考。     

Errors prediction for vector-to-raster conversion based on map load and cell size

Vector-to-raster conversion is a process accompanied with errors.The errors are classified into predicted errors before rasterization and actual errors after that.Accurate prediction of the errors is beneficial to developing reasonable rasterization technical schemes and to making products of high quality.Analyzing and establishing a quantitative relationship between the error and its affecting factors is the key to error prediction.In this study,land cover data of China at a scale of 1:250 000 were taken as an example for analyzing the relationship between rasterization errors and the density of arc length(DA),the density of polygon(DP) and the size of grid cells(SG).Significant correlations were found between the errors and DA,DP and SG.The correlation coefficient(R2) of a model established based on samples collected in a small region(Beijing) reaches 0.95,and the value of R2 is equal to 0.91 while the model was validated with samples from the whole nation.On the other hand,the R2 of a model established based on nationwide samples reaches 0.96,and R2 is equal to 0.91 while it was validated with the samples in Beijing.These models depict well the relationships between rasterization errors and their affecting factors(DA,DP and SG).The analyzing method established in this study can be applied to effectively predicting rasterization errors in other cases as well.     

An explanation for 13 consecutive day activities of Mrk 421

It is surprising to find an instance of migration in the peak positions of synchrotron spectral energy distribution components during the activity epochs of Markarian 421(Mrk 421),accompanying an orphan flare at the X-ray and GeV-TeVγ-ray bands.A geometric interpretation and standard shock or stochastic acceleration models of blazar emission have difficulty reproducing these observed behaviors.The present paper introduces a linear acceleration by integrating the reconnection electric field into the particle transport model for the observed behaviors of Mrk 421.We note that strong evidence for evolution in characteristic of multi-wavelength spectral energy distribution including shifting the peak frequency,accompanying an orphan flare at the X-ray and GeV-TeVγ-ray bands provides an important electrostatic acceleration diagnostic in a blazar jet.Assuming suitable model parameters,we apply the results of the simulation to the 13-day flaring event in March 2010 of Mrk 421,concentrating on the evolution of multiwavelength spectral energy distribution characteristic by shifting the peak frequency.It is clear that the ratio of the electric field and magnetic field strength plays an important role in temporal evolution of the peak frequency of synchrotron spectral energy distribution component.We suggest it is reasonable that the electrostatic acceleration is responsible for the evolution of multi-wavelength spectral energy distribution characteristic by shifting the peak frequency.Based on the model results,we assert that the peak frequency of the synchrotron spectral energy distribution component may signify a temporary characteristic of blazars,rather than a permanent one.     

Investigating variable stars in the open cluster NGC 1912 and its surrounding field

In this work,we studied the variable stars in the open cluster NGC 1912 based on the photometric observations and Gaia DR2 data.More than 3600 CCD frames in B,V,R filters were reduced,and we obtained the light curves that span about 63 hours.By analyzing these light curves,we detected 24 variable stars,including 16 periodic variable stars,seven eclipsing binaries and one star whose type is unclear.Among these 24 variable stars,11 are newly discovered,which are classified as sixγDoradus stars,oneδScuti star,three detached binaries and one contact binary.We also confirmed 13 previously known variable stars.Based on cluster members identified by Cantat-Gaudin et al.(2018),we inferred cluster memberships for these detected variable stars.Using Gaia DR2 data,we plotted a new color-magnitude diagram for NGC1912,and showed the nature of variable cluster members in kinematical properties and heliocentric distance.Among the 24 variable stars,seven variables are probable cluster members,which show homogeneity in kinematic characters and space position with the established cluster members.Four of the seven variable cluster members are the previously discovered stars,consisting of twoγDor stars and twoδSct stars.The remaining three variable cluster members,which are allγDor stars,are firstly detected in this work.The main physical parameters of these variable cluster members estimated from the color-magnitude diagram are log(age/yr)=8.75,[Fe/H]=-0.1,m-M=10.03 mag,and E(B-V)=0.307.     

山东巨野核桃园地区磁异常特征及找矿方向分析

山东巨野核桃园地区是鲁西南地区沉积变质型铁矿床的成矿有利靶区,利用地面高精度磁测对该地区航磁异常进行查证,圈定了磁异常区4处,选取其中1个异常区进行钻探验证,首次在山东巨野地区发现沉积变质型铁矿床,地质找矿工作取得突破性进展,同时为下一步勘查工作奠定了基础,验测结果表明,李登楼—考庄一带找矿靶区成为今后巨野核桃园地区铁矿勘查工作的首选区域。     

辽宁省温带气旋龙卷的环境参数特征

利用欧洲中期天气预报中心ERA5再分析数据,统计1979—2020年辽宁省42个温带气旋龙卷环境背景和物理量参数特征,结果表明:辽宁省温带气旋龙卷多发于温带气旋中心的西南、东南象限,与冷锋前暖区相对应,主要分布在辽河平原中西部及渤海湾沿岸,强龙卷(EF2及以上级别)占比为28.6%。风暴相对螺旋度和对流有效位能的大值区出现在气旋西南—东南象限,呈带状分布,龙卷风暴主要分布于风暴相对螺旋度大值区西北侧、对流有效位能大值区的顶端的强梯度区附近。强龙卷参数最大值达0.7,其大值区与EF2及以上级别龙卷相对应。地面冷锋和干线是温带气旋龙卷的关键触发系统,对比近气旋中心和冷锋尾部湿度垂直分布,后者所表现的高层强干侵入导致风暴产生更强的冷池,过强的下沉气流可能是龙卷产生的不利因素。温带气旋龙卷多分布于高空急流左侧气流的分流区内,对应高空强辐散区。0~3 km垂直温度递减率大值区与气旋中心附近的弱龙卷高发区有较好对应关系。     

姿态型GPS在无线电罗盘试飞中的应用

无线电罗盘是飞机常备的导航设备之一。阐述了姿态型GPS在无线电罗盘飞行试验中应用的有关问题，介绍了利用姿态型GPS鉴定无线电罗盘方位精度和作用距离的方法。