昆仑山北坡岛状冻土区西大滩大型饮用矿泉群成因分析

在对昆仑山北坡岛状冻土区西大滩大型饮用矿泉群水文地质、导水与控水断裂、水化学等方面实地调查和EH-4高频、电测深勘探的基础上,认为矿泉群的补给源为昆仑山玉珠峰一带的现代冰川底部冰雪覆盖融区水、冰雪消融水、大气降水和地表水.补给源水通过具多期活动性的F3和F4正断层组破碎带补给深层地下水.深层地下水在西倾近南北向正断层组F2及F2-1,2的导水断层破碎带富集并继续向北径流,径流至F1南倾活动性逆断层上盘时,形成富水三角区,并沿F1断层破碎带排泄出地表,是西大滩大型饮用矿泉群形成的主因.     

喀左盆地九佛堂组露头高分辨率层序地层划分

在实测106 km剖面和对喀左盆地九佛堂组沉积特征及演化进行详细研究的基础上,依据相序关系,并结合碳酸钙、油页岩的成因意义,将九佛堂组划分了 1个长期基准面旋回和7个中期基准面旋回。在长期基准面旋回内,上升期的中期基准面旋回发育以上升半旋回为主的不完全对称型中期基准面旋回,上升与下降过渡期的中期基准面旋回,则发育近完全对称的中期基准面旋回,下降期的中期基准面旋回,则发育以下降半旋回为主的不完全对称型中期基准面旋回。经过对中期基准面旋回和短期基准面旋回发育特点和形成原因的详细研究,对代表剖面进行了中期基准面旋回对比。     

A possible explanation for the electron/positron excess of ATIC/PAMELA

Results from PAMELA and ATIC indicate that the Kaluza-Klein type dark matter particles could be the annihilation source of the observed excess of electrons and positrons.Assuming the existence of a nearby black hole with 10000–100000 solar masses and a point source boost algorithm,we apply the standard propagation model and find that the results fit the data well.     

水脉泽寄主活动星系核的吸积率(英文)

水超脉泽辐射( 各向同性光度超过 10 个太阳光度) 通常在星系中心最内部的核区( 小于几个秒差距) 被发现,因而活动星系核被认为是其唯一的能量源。同其它没有检测到水脉泽辐射的活动星系核相比,水脉泽寄主活动星系核可能隐含着某种或某些特殊性质。基于此我们调研了已经公开发表的所有水脉泽源的 X 射线观测情况,得到了一个有 X 射线观测研究结果的子样本( 39 个源) 。由它们的 X 射线光度以及估算的黑洞质量,导出了它们的无量纲吸积率( logL2-10keV /LEdd,其中 L2-10keV和 LEdd分别是 2 - 10keV 的固有光度和爱丁顿光度) ; 与距离范围相当的、没有检测到水脉泽的活动星系核样本相比,发现脉泽寄主活动星系核有较高的吸积率。进一步分析比较这两个活动星系核样本的质量吸积率,也发现类似的趋势。此外,为了探索吸积率和水脉泽辐射间可能的内在联系,我们对它们的脉泽光度和吸积率进行了统计分析,然而结果显示二者之间没有明显的相关性。     

Solar Intranetwork Magnetic Elements: Evolution and Lifetime

Based on Hinode SOT/NFI observations with greatly improved spatial and temporal resolution and polarization sensitivity, the lifestory of the intranetwork (IN) magnetic elements are explored in a solar quiet region. A total of 2282 IN elements are followed from their appearance to disappearance and their fluxes measured. By tracing individual IN elements their lifetimes are obtained, which fall in the range from 1 to 20 min. The average lifetime is 2.9±2.0 min. The observed lifetime distribution is well represented by an exponential function. Therefore, the e-fold characteristic lifetime is determined by a least-square fitting to the observations, which is 2.1±0.3 min. The lifetime of IN elements is correlated closely with their flux. The evolution of IN elements is described according to the forms of their birth and disappearance. Based on the lifetime and flux obtained from the new observations, it is estimated that the IN elements have the capacity of heating the corona with a power of 2.1×10²⁸ erg s⁻¹ for the whole Sun.     

扩展SSH Hubbard模型的晶格振动矩阵

在计及最近邻电子相互作用的扩展ＳＳＨＨｕｂｂａｒｄ模型时，得到了晶格振动矩阵，它对电子的正负自旋态对称和非对称的各类非线性元激发情形均适用。     

The Faraday rotation of sunspots

In this paper the numerical solutions of the Unno-Beckers's equations for the magneto-sensitive line Fei 5250.216 are used to demonstrate the importance and role of Faraday rotation in sunspot magnetic fields and to study the influence of this effect on the measurements of the azimuth of the transverse field. We propose a method to determine the intrinsic direction of the transverse field with the observed azimuthal angle of the plane of linear polarization.     

Study on polycyclic aromatic hydrocarbons（PAHs） contents and sources in the surface so~l or l-lmznou City, South China, based on multivariate statistics analysis

Studies of polycyclic aromatic hydrocarbons (PAHs) in the surface soil were conducted in Huizhou City, which is located in the Pearl River Delta, South China. Sixteen PAHs in 42 soil samples were detected. The results showed that 4 components of PAHs were detectable in all soil samples, and other 12 components were also detectable to some extent. The total PAHs contents range from 35.40 to 534.5 μg/kg with the mean value of 123.09 μg/kg. Soil in Huizhou was slightly polluted by PAHs according to Maliszewska-Kordybach’s study. It can be confirmed that the increase of PAHs contents in the surface soil of Huizhou City is closely connected to human activities. Multivariate analysis was also made in this study. Principal component analysis was used to constrain their origins, and 3 principal components (PCs) were extracted. The results showed that coal combustion and oil spilling made the major contributions to PAHs. Cluster analysis was made and 16 priority PAHs were classified as 4 sorts, and the result revealed the differences in environmental behavior, chemical properties and sources of PAHs.     

深层裂缝性储层防漏堵漏实验评价研究

深层裂缝性气藏具有异常高压、高产等特点,钻井完井过程中易出现又喷又漏等复杂事故,因此需做好“防漏为主、堵漏为辅”的防漏堵漏措施。通过全尺寸堵漏装置进行了高压静态、动态模拟堵漏实验,优选配方组合,并系统评价了防漏、堵漏配方的封堵能力、承压能力以及酸溶性,评价研究出的防漏堵漏配方,具有酸溶率高、堵塞强度高、返排效果好等特点,为防漏、堵漏方案现场实施提供依据。     

大脑中动脉狭窄程度与脑梗死前期CT灌注参数的相关性

目的:探讨单侧大脑中动脉(MCA)狭窄程度与脑梗死前期CT灌注(CTP)参数的关系,并分析梗死前期血管表面通透性(PS)的变化。方法:回顾性分析我院2018年7月1日至2019年10月1日期间经头颈部CTA诊断单侧MCA狭窄患者108例,观察CTP成像特点,测量各组患侧、镜像侧剩余函数达峰时间(TMax)、平均通过时间(MTT)、脑血流量(CBF)、脑血容量(CBV)以及表面通透性(PS),并计算各灌注参数的相对值(患侧/镜像侧),分析单侧大脑中动脉狭窄程度与脑梗死前期CT灌注参数的相关性。结果:①108例单侧大脑中动脉狭窄患者中39例出现灌注异常,不同程度血管狭窄的灌注分期差异具有统计学意义(P=0.009)。单侧大脑中动脉狭窄程度与灌注异常分期呈中等正相关(r=0.557,P=0.000)。②单侧大脑中动脉不同程度狭窄组间rCBF值、rMTT值差异有统计学意义(P<0.05),而rCBV值、r TMax值差异无统计学意义(P>0.05)。单侧大脑中动脉狭窄程度与rTMax值、rMTT值呈正相关(分别为r=0.458,P=0.003,r=0.765,P=0.000),与rCBF呈负相关相关(r=-0.600,P=0.000),而狭窄程度与rCBV值无明显相关性。③Ⅱa、Ⅱb期患者患侧与镜像侧PS绝对值差异有统计学意义(P<0.05),Ⅱa、Ⅱb期患者组间PS相对值差异没有统计学意义(P>0.05)。结论:单侧MCA狭窄程度与脑梗死前期分期具有一定相关性,单侧MCA狭窄程度越严重,rTMax、rMTT值越大,rCBF越小;在脑梗死前期的II期出现血管表面通透性升高的改变。