A spectroscopic study of DD UMa: Ursa Major group member and candidate for BRITE     

A. Elmasl?  L. Fossati 《New Astronomy》2012,17(2):221-226

The Ursa Major group is a nearby stellar supercluster which, while not gravitationally bound, is defined by co-moving members. DD UMa is a δ Scuti star whose membership in the Ursa Major group is unclear.The objective of this study is to confirm the membership of DD UMa in the Ursa Major group, as well as perform a detailed spectral analysis of the star. Since DD UMa is a low-amplitude δ Scuti star, we performed a frequency analysis. We determined fundamental parameters, chemical abundances, and derive a mass and age for the star.For this study we observed DD UMa at the Okayama Astrophysical Observatory with the high-resolution spectrograph HIDES, between the 27th of February and the 4th March, 2009. Additional observations were extracted from the ELODIE archive in order to expand our abundance analysis. Group membership of DD UMa was assessed by examining the velocity of the star in Galactic coordinates. Pulsational frequencies were determined by examining line profile variability in the HIDES spectra. Stellar fundamental parameters and chemical abundances were derived by fitting synthetic spectra to both the HIDES and ELODIE observations.DD UMa is found to be a member of the extended stream of the Ursa Major group, based on the space motion of the star. This is supported by the chemical abundances of the star being consistent with those of Ursa Major group members. The star is found to be chemically solar, with T_eff = 7450 ± 150 K and logg = 3.98 ± 0.2. We found pulsational frequencies of 9.4 and 15.0 c/d. While these frequencies are insufficient to perform an asteroseismic study, DD UMa is a good bright star candidate for future study by the BRITE-constellation.  相似文献   

非开挖施工前的管道探测方法     

吴萧 《岩土钻凿工程》2012,(2):122-124

只有在非开挖施工前探明了地下管线的分布情况,才能正确地制定施工方案,以防止对已有的地下管线造成破坏,引起人员伤亡和重大财产损失。通过对传统的和在当今比较前沿的几种地下管道探测方法做出介绍,旨在为施工人员在地下管道探测作业时提供更多的选择。  相似文献   

基于ANSYS的黄土高边坡开挖卸荷稳定性分析   总被引：1，自引：0，他引：1  

温笃武  谢婉丽  刘强  王庆满 《地下水》2012,(3):189-191

基于ANSYS软件的岩土分析模块,利用强度折减模拟边坡由稳定状态到不稳定,得到安全系数;利用网格划分后杀死单元模拟边坡开挖卸荷状态,分析其稳定性的变化,其边坡位移与监测结果基本一致。  相似文献   

华北克拉通岩石圈三维密度结构   总被引：6，自引：4，他引：2       下载免费PDF全文

王新胜  方剑  许厚泽  郑伟 《地球物理学报》2012,55(4):1154-1160

显生宙以来华北克拉通岩石圈遭到破坏,这一现象的科学问题已受到世界地学家广泛关注.本文首先将地震层析成像反演得到的P波速度扰动转化为密度扰动,以此作为初始密度模型,然后利用布格重力异常反演得到了华北克拉通岩石圈高分辨三维密度结构.为了避开大型稀疏矩阵求逆计算,提高计算效率,我们将代数重构技术用于密度反演解算.反演结果表明:华北克拉通岩石圈密度在横向和纵向上均存在明显的不均匀性,密度分布形态与地表构造格局有很好的相关性;研究区地壳整体表现为低密度异常,地壳以下岩石圈部分则以高密度异常为主;鄂尔多斯块体地壳范围内以低密度异常为主,80~120 km深度上为呈南北两端集中分布的高密度异常,并分别与秦岭造山带和阴山造山带的高密度异常分布相连,这暗示了鄂尔多斯块体可能受到了来自其南北两端造山带深部动力学过程的影响;80~120 km深度上,华北克拉通东部地区呈现出显著的南北向非均匀的高密度异常,这表明遭到破坏后该地区上地幔物质分布具有强烈的南北向非均匀性.  相似文献   

1980—2014年中国台风大风和台风极端大风的变化     

陆逸  朱伟军  任福民  王昕 《气候变化研究进展》2016,12(5):413-421

基于1980—2014中国670站日最大风速资料,利用改进的客观天气图分析法（OSAT）分离出中国陆地的台风大风（6级以上,≥10.8 m/s）,并定义了台风极端大风,进而研究了台风大风和台风极端大风的变化特征。分析表明：在地理分布上,台风大风年均日数和占比均自海岸线向内陆迅速减小,在海南、华南和东南沿海省份以及江苏南部,台风大风占比一般为30%～70%;台风极端大风年均日数大值主要分布在沿海省市（除河北和天津）,特别是华东和华南沿海,局部地区台风极端大风日数占比达100%。从季节变化看,在台风活跃的7—9月,中国台风极端大风频次总体上超过了季风极端大风;就全国而言,当阈值从最低值（11.5 m/s）提升至12级（32.7 m/s）时,台风极端大风频数占比则从12%急剧攀升至77%。1980—2014年,中国台风大风和台风极端大风年日数均显著减少,而台风极端大风年平均强度增强;这期间引起中国台风大风和台风极端大风的台风频数均显著减少,但引起台风极端大风的台风在生命期和影响期的平均强度均显著增强,这可能是上述显著变化特征的主要原因。  相似文献   

一种制造高精度水准尺的新型工艺     

张君  郭彦珍 《测绘学院学报》1999,(2)

分析了目前我国生产水准尺的工艺现状, 指出了造成水准尺精度长期得不到提高的原因。提出了一种使用感光成像法制造高精度水准尺的制造工艺。  相似文献   

复杂勘探目标区岩性预测技术及其在海拉尔盆地乌南地区的应用     

王江  张宏  邵红君 《海相油气地质》2010,15(4)

海拉尔盆地乌尔逊凹陷南部地区构造和断裂复杂,多物源,短物源,相变快,因而导致下白垩统南屯组岩性有利目标区预测难度大。根据层序地层学和坡折带理论,以地震资料为基础,建立了一套新的地震精细解释、复杂勘探目标区岩性体识别及三维可视化刻画等全三维地震解释技术体系。认为乌东斜坡发育三个坡折带,第三坡折带下倾方向和第二坡折带具备形成岩性油气藏的地质条件,应用频谱分析和三维可视化技术在乌东斜坡带南屯组识别有利扇体10个,面积145km2,部署探井5口,其中4口获工业性油流,1口获低产工业性油流,探井符合率100%。  相似文献   

FT-IR microspectroscopy of extraterrestrial dust grains: Comparison of measurement techniques     

A. Morlok  M. Köhler  Monica M. Grady 《Planetary and Space Science》2006,54(6):599-611

Identification of astronomical dust composition rests on comparison of Infrared (IR) spectra with standard laboratory spectra; frequently, however, a single mineralogical composition is assumed for spectral matching. Advances in laboratory instrumentation have enabled very precise IR spectra to be measured on single grains and zones within grains; with a more complete set of spectral data for planetary dust, better compositional matches will be achieved for astronomical dust. We have compared several FT-IR spectroscopy techniques (open path transmission spectroscopy and diffuse reflectance spectroscopy of powders; microspectroscopy of single grains and powders and ATR spectroscopy of thin sections) to determine their utility for the direct measurement of the mid-IR spectra of small amounts of extraterrestrial grains. We have focussed our investigation on the spectra of the olivine series of silicates, (Mg,Fe)₂SiO₄, a species frequently identified as one of the major constituents of interstellar dust. The positions of three characteristic SiO₄ stretching bands at ∼10.4, 11.3 and 12 μm were measured for comparison of the techniques. All methods gave satisfactory results, although care must be taken to guard against artefacts from sample thickness and orientation effects. Single grains hand-picked from meteorites can be analysed, but results are inaccurate if the grain size is too large (>1-10 μm). Spectra for single grains also show variations that arise from sample orientation effects. Once the analytical artefacts are taken into account, we found that measurement of powder with a diamond compression cell is best suited for the analysis of small amounts of materials.  相似文献   

Data replenishment of five moderate earthquake sequences in Japan,with semi-automatic cluster selection          下载免费PDF全文

Yi Zheng  Bogdan Enescu  Jiancang Zhuang  Coleman Yu 《地震科学（英文版）》2021,34(4):310-322

Missing early aftershocks following relatively large or moderate earthquakes can cause significant bias in the analysis of seismic catalogs. In this paper, we systematically address the aftershock missing problem for five earthquake sequences associated with moderate-size events that occurred inland Japan, by using a stochastic replenishing method. The method is based on the notion that if a point process (e.g., earthquake sequence) with time-independent marks (e.g., magnitudes) is completely observed, it can be transformed into a homogeneous Poisson process by a bi-scale empirical transformation. We use the Japan Meteorological Agency (JMA) earthquake catalog to select the aftershock data and replenish the missing early events using the later complete part of each aftershock sequence. The time windows for each sequence span from 6 months before the mainshock to three months after. The semi-automatic spatial selection uses a clustering method for the epicentral selection of earthquakes. The results obtained for the original JMA catalog and replenished datasets are compared to get insight into the biases that the missing early aftershocks may cause on the Omori-Utsu law parameters’ estimation, characterizing the aftershock decay with time from the mainshock. We have also compared the Omori-Utsu law parameter estimates for two datasets following the same mainshock; the first dataset is the replenished sequence, while the second dataset has been obtained by waveform-based analysis to detect early aftershocks that are not recorded in the JMA catalog. Our results demonstrate that the Omori-Utsu law parameters estimated for the replenished datasets are robust with respect to the threshold magnitude used for the analyzed datasets. Even when using aftershock time windows as short as three days, the replenished datasets provide stable Omori-Utsu law parameter estimations. The p-values for all the analyzed sequences are about 1.1 and c-values are significantly smaller compared to those of original datasets. Our findings prove that the replenishment method is a fast, reliable approach to address the missing aftershock problem.  相似文献   

Quantitative estimates of temperature and precipitation changes over the last millennium from pollen and lake-level data at Lake Joux, Swiss Jura Mountains     

Michel Magny  Odile Peyron  Boris Vannière  Bruno Vermot-Desroches 《Quaternary Research》2011,75(1):45-54

This paper presents quantitative climate estimates for the last millennium, using a multi-proxy approach with pollen and lake-level data from Lake Joux (Swiss Jura Mountains). The climate reconstruction, based on the Modern Analogue Technique, indicates warmer and drier conditions during the Medieval Warm Period (MWP). MWP was preceded by a short-lived cold humid event around AD 1060, and followed by a rapid return around AD 1400 to cooler and wetter conditions which generally characterize the Little Ice Age (LIA). Around AD 1450 (solar Spörer minimum), the LIA attained a temperature minimum and a summer precipitation maximum. The solar Maunder minimum around AD 1690 corresponded at Joux to rather mild temperatures but maximal annual precipitation. These results generally agree with other records from neighbouring Alpine regions. However, there are differences in the timing of the LIA temperature minimum depending on the proxy and/or the method used for the reconstruction. As a working hypothesis, the hydrological signal associated with the MWP and LIA oscillations at Lake Joux may have been mainly driven by a shift around AD 1400 from positive to negative NAO modes in response to variations in solar irradiance possibly coupled with changes in the Atlantic meridional overturning circulation.  相似文献