Flare-induced signals in polarization measurements during the X2.6 flare on 2005 January 15

Flare-induced signals in polarization measurements which were manifested as apparent polarity reversal in magnetograms have been reported since 1981. We are motivated to further quantify the phenomenon by asking two questions: can we distinguish the flare-induced signals from real magnetic changes during flares, and what we can learn about flare energy release from the flare-induced signals? We select the X2.6 flare that occurred on 2005 January 15, for further study. The flare took place in NOAA active re-gion (AR) 10720 at approximately the central meridian, which makes the interpretation of the vector magnetograms less ambiguous. We have identified that flare-induced signals during this flare appeared in six zones. The zones are located within an average distance of 5 Mm from their weight center to the main magnetic neutral line, have an average size of (0.6±0.4)×1017 cm2, duration of 13±4 min, and flux density change of 181±125 G in the area of reversed polarity. The following new facts have been revealed by this study: (1) the flare-induced signal is also seen in the transverse magnetograms but with smaller magnitude, e.g., about 50 G; (2) the flare-induced signal mainly manifests itself as apparent polarity reversal, but the signal starts and ends as a weakening of flux density; (3) The flare-induced signals appear in phase with the peaks of hard X-ray emission as observed by the Ramaty High Energy Solar Spectroscopic lmager (RHESSI), and mostly trace the position of RHESSI hard X-ray footpoint sources. (4) in four zones, it takes place cotemporally with real magnetic changes which persist after the flare. Only for the other two zones does the flux density recover to the pre-flare level immediately after the flare.The physical implications of the flare-induced signal are discussed in view of its relevance to the non-thermal electron precipitation and primary energy release in the flare.     

Pressure dependence of viscosity of rhyolitic melts

Viscosity of silicate melts is a critical property for understanding volcanic and igneous processes in the Earth. We investigate the pressure effect on the viscosity of rhyolitic melts using two methods: indirect viscosity inference from hydrous species reaction in melts using a piston cylinder at pressures up to 2.8 GPa and direct viscosity measurement by parallel-plate creep viscometer in an internally-heated pressure vessel at pressures up to 0.4 GPa. Comparison of viscosities of a rhyolitic melt with 0.8 wt% water at 0.4 GPa shows that both methods give consistent results. In the indirect method, viscosities of hydrous rhyolitic melts were inferred based on the kinetics of hydrous species reaction in the melt upon cooling (i.e., the equivalence of rheologically defined glass transition temperature and chemically defined apparent equilibrium temperature). The cooling experiments were carried out in a piston-cylinder apparatus using hydrous rhyolitic samples with 0.8-4 wt% water. Cooling rates of the kinetic experiments varied from 0.1 K/s to 100 K/s; hence the range of viscosity inferred from this method covers 3 orders of magnitude. The data from this method show that viscosity increases with increasing pressure from 1 GPa to 3 GPa for hydrous rhyolitic melts with water content ?0.8 wt% in the high viscosity range. We also measured viscosity of rhyolitic melt with 0.13 wt% water using the parallel-plate viscometer at pressures 0.2 and 0.4 GPa in an internally-heated pressure vessel. The data show that viscosity of rhyolitic melt with 0.13 wt% water decreases with increasing pressure. Combining our new data with literature data, we develop a viscosity model of rhyolitic melts as a function of temperature, pressure and water content.     

粉晶X射线衍射法在岩石学和矿物学研究中的应用

X射线衍射是测定物质结构的主要分析手段,广泛应用于物理学、化学、医药学、金属学、材料学、工程技术学、地质学和矿物学。文章综述了粉晶X射线衍射法在造岩矿物、黏土矿物、岩组学、类质同象和结晶度的测定等领域发挥的重要作用。随着测量技术的发展,粉晶X射线衍射在矿物结晶过程中的研究、矿物表面研究、矿物定量相分析和矿物晶体结构测定方面均有新的应用。     

大型凹陷向斜区油气倒灌式成藏——以松辽盆地三肇凹陷扶杨油层为例

三肇凹陷扶杨油层为典型大型凹陷向斜区油气倒灌式成藏,利用300条地震剖面、825口井曲线、11口井岩芯和探评井试油资料对扶杨油层断层特征及运动期次、油气下排深度、储层沉积特征等油气成藏主控因素综合研究表明：T2断层受控于基底断层、下部火山口、斜向拉张和伸展量差异四种因素具有平面密集成带、剖面“似花状”组合特征,且油气成藏期活动的油源断层多数为断层密集带边界断层;理论计算超压驱动油气下排深度和实际油底包络面统计扶杨油层含油厚度约为200m;重矿物分析扶杨油层主要受北部拜泉—青冈和西南保康物源影响,两物源在徐家围子地区交汇后向东流出;沉积微相揭示扶杨油层发育向上逐渐退积的河控浅水三角洲沉积体系,顶部为三角洲前缘亚相,中—下部为三角洲分流平原亚相,其中扶Ⅰ7—扶Ⅱ1小层为水退最大期,是油气富集主要层位。明水组末期青山口组源岩达到生油高峰,油气在超压作用下沿开启的断层密集带边界断层幕式下排后沿两侧上升盘河道砂体做短距离侧向运移,即断层密集带两侧地垒或断阶块为油气富集区,而断层密集带内多为地堑式组合,不利于油气聚集,在成藏模式指导下刻画出47个油气富集目标区,为松辽盆地北部扶杨油层下一步的勘探与开发指明了方向。     

大陆地壳深熔作用中自由水的贡献——以高喜马拉雅淡色花岗岩为例

高喜马拉雅淡色花岗岩是印度与亚洲板块碰撞过程中,地壳深熔作用的产物.尽管自由水对高喜马拉雅淡色花岗岩形成的重要性已被多次报导,但仍存在许多争议.本研究汇编了高喜马拉雅淡色花岗岩的全岩地球化学数据,证明高喜马拉雅淡色花岗岩可以由脱水熔融形成和水致熔融形成.进一步通过热力学模拟获得锆石结晶,并与锆石Ti温度计比较,限定了不...     

无/缺水下地形数据的高原堰塞湖水量遥感估算

水量遥感动态监测对于高原堰塞湖风险评估、预报预警和处置决策等具有重要意义。针对高原无资料或缺资料区,充分利用空天遥感技术,文章提出了一种无/缺水下地形数据的高原堰塞湖水量遥感定量估算方法。该方法首先通过遥感水域面积提取,获取堰塞湖淹没空间范围;进而采用不规则复杂多边形中线定位算法,确定堰塞湖中心线位置;然后基于河道中心特定点高程信息,结合局部河道比降估算,生成堰塞湖水下地形河道中线约束因子;再根据河道边坡高程信息和水下地形约束因子自适应拟合出局部堰塞河道的水下未知地形;最后通过三维曲面离散积分实现堰塞湖水量遥感动态定量估算。实验以东帕米尔高原的萨雷兹堰塞湖为研究区,展开遥感水量调查与局部验证研究,结果表明:萨雷兹堰塞湖当前水域面积约为89.09 km²,水量约为162.49亿m³;这一结果与专家预估的水资源量155—165亿m³基本吻合。经局部模拟实验精度对比验证,模拟结果与实际数据动态误差总体控制在10%以内,相关系数达到0.95(P<0.01,双尾),进一步证明了算法的鲁棒性和估算结果的可信度。为无/缺水下地形数据的高原堰塞湖水量遥感估算提供了一种有效的方法,实现了水下地形未知的高原堰塞湖水量遥感快速反演与定量测算。     

MERSI和MODIS卫星监测京津冀及周边地区PM2.5浓度

京津冀及周边地区是中国PM_(2.5)污染最重的区域之一,利用卫星遥感技术监测大范围的PM_(2.5)时空分布变化是一种先进的重要手段。本研究首先基于暗像元算法利用FY-3B/MERSI与AQUA/MODIS对京津冀及周边区域进行了遥感AOT反演和验证分析;然后,引入气象资料和地面观测资料利用GWR模型反演了区域PM_(2.5)浓度,并对遥感反演结果进行了交叉验证评估,综合对比分析了MERSI和MODIS的气溶胶及PM_(2.5)遥感监测能力;最后,利用MERSI数据对2017年第一季度京津冀及周边区域的PM_(2.5)月均浓度时空分布变化情况进行了初步探索分析。结果表明:FY-3B/MERSI在气溶胶及PM_(2.5)遥感监测能力方面略优于AQUA/MODIS,MERSI反演的1 km分辨率AOT和PM_(2.5)与地面站点实测结果的决定系数R2分别为0.76μg/m~3和0.79μg/m~3,均方根误差分别为0.26μg/m~3和28μg/m~3,平均绝对误差分别为0.16μg/m~3和15μg/m~3,能基本满足对京津冀及周边区域PM_(2.5)的精细化监测需要。2017年第一季度京津冀及周边区域PM_(2.5)月均浓度遥感监测结果表明该区域的PM_(2.5)空间分布格局与地形地貌关系密切,高值区整体上沿太行山脉成带成片;从时间变化来看,1—3月呈逐月下降的趋势,其中3月份PM_(2.5)区域浓度较1月和2月有大幅下降。这说明FY-3\MERSI遥感反演产品能为环境质量监测和环境管理工作效果评估提供有效参考,本研究对国产卫星在大气环境遥感业务中的大力发展应用有重要参考意义。     

高速公路用地地籍调查方法和精度研究

介绍高速公路用地的权属调查和地籍测量方法,根据高速公路用地特点,重点讨论了确定高速公路地籍测量精度指标问题,得出高速公路宗地界址点精度统一采用&#177;0．3m比较适宜的结论。最后介绍了RTK技术在高速公路地籍测量的应用情况。