阿勒泰地区植被覆盖度及ET对气温变化的响应

研究气温对植被覆盖度和ET (Evapotranspiration,ET)的影响,对干旱区应对气候变化、维系生态系统稳定具有重要意义。基于阿勒泰地区及周边7个气象站,CRU数据集中的气温数据及MODIS ET数据,采用Mann-Kendall非参数检验、植被盖度反演等方法,对阿勒泰地区气温变化对植被覆盖度及ET的影响进行了研究。结果表明：（1）在1901—2016年过去的116 a间,阿勒泰地区年平均气温以0.18 ℃·(10 a)^-1速率增加,在1982年由突变前的2.2 ℃增加到突变后的3.5 ℃。（2）2000—2017年阿勒泰地区植被覆盖度变化的空间差异明显,植被覆盖度增加的面积与降低的面积总体相当;全区66.71%的区域植被覆盖度变化与气温呈负相关,而呈正相关的比例仅占18.55%,且全区气温变暖而盖度降低区域的占比达31.71%。（3）2000—2016年阿勒泰地区ET总体呈降低趋势,整个区域61.65%的面积温度降低、ET降低,而19.92%的区域表现为温度增加而植被ET降低。     

2000-2015年三江平原主要作物需水量征及影响因素分析

全生育期内作物需水量的研究是农业水资源有效利用和进行合理灌溉的重要依据。基于三江平原22个气象站点2000—2015年逐日气象观测资料及中国区域地面气象要素数据集,利用国际粮农组织 （FAO）Penman-Monteith模型和分段单值平均作物系数法,分别对三江平原水稻、玉米和大豆的作物需水量进行计算,分析作物需水量年际变化特征,采用通径分析法研究作物需水量的变化成因。结果表明：（1）三江平原16 a来年均参考作物蒸散量为537.4 mm,日均为 3.5 mm,呈波动减少趋势。（2）生长季内,水稻在分蘖期需水量最大,为177.1 mm,玉米在七叶期需水量最大,为99.7 mm,大豆在结荚期需水量最大,为96.1 mm;水稻、玉米和大豆的净灌溉需水量分别为195.4 mm、130.8 mm和72.2 mm,对灌溉的依赖程度水稻>玉米>大豆。（3）由通径分析结果可知,三江平原作物需水量的主要影响因素为净辐射、气温和日照时数。     

加味栝楼薤白汤治疗痰瘀互结型慢性稳定型心绞痛30例

目的：观察加味栝楼薤白汤治疗痰瘀互结型慢性稳定型心绞痛的临床疗效。方法：将60例痰瘀互结型慢性稳定型心绞痛患者随机分为治疗组和对照组,每组各30例。2组均予以口服阿司匹林肠溶片治疗,治疗组在此基础上加服加味栝楼薤白汤治疗,对照组在此基础上加服脑心清片治疗。比较2组患者中医证候积分、西雅图心绞痛量表积分、中医证候疗效与心绞痛疗效。结果：中医证候疗效、心绞痛疗效的总有效率治疗组分别90.0%、86.7%,对照组分别为73.3%、66.7%,2组比较,差异均有统计学意义（P<0.05）;2组患者中医证候积分、西雅图心绞痛量表积分治疗前后组内比较及治疗后组间比较,差异均有统计学意义（P<0.05）。结论：选用加味栝楼薤白汤治疗痰瘀互结型慢性稳定型心绞痛可有效缓解患者胸闷、胸痛、心悸、气短等症状,提高中医证候疗效和心绞痛疗效,并可有效改善躯体受限活动的程度,值得临床推广。     

有机质对海底沉积物中粘土矿物X射线衍射分析结果的影响

X射线衍射法广泛应用于分析粘土矿物的含量和结晶特征,由于粘土矿物易与有机质结合形成有机-粘土复合体,是否去除有机质对分析结果有很大影响,实验结果表明影响最大的是伊-蒙混层矿物(含蒙脱石)和伊利石的含量,为得到可靠实验数据,必须重视对样品的前处理工作,对不同批次样品应该保持一致的处理程序。     

运用ADC模型结合层次分析法评估LMAUV系统效能

基于WSEIAC给出的武器系统效能定义和ADC基本模型,针对LM AUV作战使用特点,对可用度、可信度基本函数进行完善,并运用模糊层次分析法和乘法模型得出系统能力向量,建立LM AUV系统效能评估模型;最后,结合算例结果分析,验证该方法评估LM AUV系统效能的有效性。     

北斗星地双向时频传递与广广播钟差精度分析

与其他卫星导航系统不同,北斗卫星导航系统采用星地双向时间比对技术,直接测量卫星钟相对于地面保持的系统时间的钟差,并用于广播电文钟差参数的建模。讨论了电离层延迟误差、卫星相位中心误差等不同误差源对不同类型卫星双向时间同步卫星钟差精度的影响。实测数据分析结果表明,星地双向卫星钟差内符合精度(RMS)优于0.15 ns。利用双向卫星钟差序列,对广播星历钟差参数预报精度进行了分析,统计结果显示广播电文钟差参数预报1 h,精度在2 ns以内,移动卫星刚入境时,钟差参数预报6 h误差可达10 ns。     

巡天项目中的白矮星搜寻

首先,描述了白矮星的颜色特点和光谱型分类。白矮星是大多数恒星的终极状态,它会随着时间的推移而逐渐冷却。根据表面大气成分,它被划分成DA和DB等不同的光谱型。对某一颗白矮星来说,其光谱型分类可能会随着时间的推移而发生变化,这主要是由于其大气包层中的元素含量被对流过程改变引起的。为了对各类光谱型有更深入的研究,样本的完备性不可或缺。得益于近十几年来大型巡天项目的开展(如斯隆数字巡天、郭守敬望远镜的光谱巡天等),目前通过光谱证认的白矮星已超过4×10~4颗,其中绝大多数是H主导的DA型白矮星,另外还包含2 000多颗He主导的DB白矮星。此外,GALEX项目和GAIA卫星分别提供了有价值的白矮星紫外数据、空间位置和速度等信息。这些数据和信息对于白矮星的研究工作起到了非常大的促进作用。随后,对白矮星的大气参数、质量和运动学等内容作了简单的总结。人们利用模板匹配测量了绝大多数已知白矮星的大气参数,并获得了DB型白矮星的有效温度与紫外颜色间的线性关系。基于斯隆数字巡天的光谱数据,白矮星的质量分布和质量-半径关系也得到了较深入的研究。小质量白矮星具有较大的速度弥散,而大质量的则相反。最后,讨论了白矮星的形成和演化机制,这些机制都是基于现有的理论模型得到的。随着巡天项目中白矮星样本的增加,现有的模型会逐渐被修正和完善,新的模型也将随之建立。     

Northwest Africa 11024—A heated and dehydrated unique carbonaceous (CM) chondrite

Based on the high abundance of fine‐grained material and its dark appearance, NWA 11024 was recognized as a CM chondrite, which is also confirmed by oxygen isotope measurements. But contrary to known CM chondrites, the typical phases indicating aqueous alteration (e.g., phyllosilicates, carbonates) are missing. Using multiple analytical techniques, this study reveals the differences and similarities to known CM chondrites and will discuss the possibility that NWA 11024 is the first type 3 CM chondrite. During the investigation, two texturally apparent tochilinite–cronstedtite intergrowths were identified within two thin sections. However, the former phyllosilicates were recrystallized to Fe‐rich olivine during a heating event without changing the textural appearance. A peak temperature of 400–600 °C is estimated, which is not high enough to destroy or recrystallize calcite grains. Thus, calcites were never constituents of the mineral paragenesis. Another remarkable feature of NWA 11024 is the occurrence of unknown clot‐like inclusions (UCLIs) within fine‐grained rims, which are unique in this clarity. Their density and S concentration are significantly higher than of the surrounding fine‐grained rim and UCLIs can be seen as primary objects that were not formed by secondary alteration processes inside the rims. Similarities to chondritic and cometary interplanetary dust particles suggest an ice‐rich first‐generation planetesimal for their origin. In the earliest evolution, NWA 11024 experienced the lowest degree of aqueous alteration of all known CM chondrites and subsequently, a heating event dehydrated the sample. We suggest to classify the meteorite NWA 11024 as the first type 3 CM chondrite similar to the classification of CV3 chondrites (like Allende) that could also have lost their matrix phyllosilicates by thermal dehydration.     

(U‐Th)/He zircon dating of Chesapeake Bay distal impact ejecta from ODP site 1073

Single crystal (U‐Th)/He dating has been undertaken on 21 detrital zircon grains extracted from a core sample from Ocean Drilling Project (ODP) site 1073, which is located ~390 km northeast of the center of the Chesapeake Bay impact structure. Optical and electron imaging in combination with energy dispersive X‐ray microanalysis (EDS) of zircon grains from this late Eocene sediment shows clear evidence of shock metamorphism in some zircon grains, which suggests that these shocked zircon crystals are distal ejecta from the formation of the ~40 km diameter Chesapeake Bay impact structure. (U‐Th/He) dates for zircon crystals from this sediment range from 33.49 ± 0.94 to 305.1 ± 8.6 Ma (2σ), implying crystal‐to‐crystal variability in the degree of impact‐related resetting of (U‐Th)/He systematics and a range of different possible sources. The two youngest zircon grains yield an inverse‐variance weighted mean (U‐Th)/He age of 33.99 ± 0.71 Ma (2σ uncertainties n = 2; mean square weighted deviation = 2.6; probability [P] = 11%), which is interpreted to be the (U‐Th)/He age of formation of the Chesapeake Bay impact structure. This age is in agreement with K/Ar, ⁴⁰Ar/³⁹Ar, and fission track dates for tektites from the North American strewn field, which have been interpreted as associated with the Chesapeake Bay impact event.