川西坳陷中段新场地区天然气研究及气源对比

经过大量学者多年的研究总结,川西坳陷中段新场地区具备良好的生、储、盖等成藏组合。结合地质背景及碳同位素、轻烃的研究,认为新场地区天然气主要是Ⅲ型干酪根的煤型气,气藏主要分布在上三叠系的须二段和须四段,以及中侏罗系、上侏罗系地层中。     

Multi-band Solar Full-disk Extreme Ultraviolet Imager

Solar Extreme Ultraviolet (EUV) imaging observation is an important measure for the researches of solar activities and coronal plasma physics. But the traditional EUV imager and spectrograph can hardly achieve simultaneously the high spectral resolution and wide field-of-view of solar imaging. This paper has designed a new type of solar EUV multi-band imager, by adopting a kind of slitless grating and grazing incidence structure, it can realize the solar full-disk imaging of high spectral and spatial resolution. The field-of-view of the imager can be as broad as 47′. The spectral resolution is 2×10^?3nm per pixel, and the spatial resolution is 1.4′ per pixel. The temporal resolution of the solar full-disk is better than 60 s. The analysis of the solar full-disk spectral image and system response shows that the imager can observe the morphological evolutions of various solar activities, and can provide more comprehensive data for the researches of solar physics and space weather forecast.     

X-ray activity from different types of stars

X-ray emission is an important indicator of stellar activity. In this paper, we study stellar Xray activity using the XMM-Newton and LAMOST data for different types of stars. We provide a sample including 1259 X-ray-emitting stars, of which 1090 have accurate stellar parameter estimations. Our sample size is much larger than those used in previous works. We find a bimodal distribution of the X-ray to optical flux ratio(log(fX/fV)) for G and K stars. We interpret that this bimodality is due to two subpopulations with different coronal heating rates. Furthermore, using the full widths at half maxima calculated from Hα and Hβ lines, we show that these stars in the inactive peaks have smaller rotational velocities. This is consistent with the magnetic dynamo theory that presumes stars with low rotational velocities have low levels of stellar activity. We also examine the correlation between log(fX/fV) and luminosity of the excess emission in the Hα line, and find a tight relation between the coronal and chromospheric activity indicators.     

地质雷达方法在上海市轨道交通明珠线工程中的应用

地质雷达方法在上海市轨道交通明珠线工程中的应用表明,此方法在探测地下障碍物中能依靠雷达图象识别其类型、材质、深度等,有利于快速、准确定位,有一定的优越性。     

HD 104237,εCha和HD 100546的演化状态

根据Ｈｉｐｐａｒｃｏｓ的资料和ＴＤ－１对εＣｈａ和ＨＤ１００５４６的紫外观测资料讨论了εＣｈａ、ＨＤ１０４２３７和ＨＤ１００５４６在赫罗图上的位置以及它们的演化状态．     

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。     

Investigation of the correlation between morphology and luminosity for two classes of main galaxies

Using an apparent-magnitude limited Main galaxy sample of the Sloan Digital Sky Survey Data Release 7(SDSS DR7), we investigate the correlation between morphologies and luminosity for the Main galaxy sample. Our Main galaxy sample is divided into two classes: Main galaxies only with TARGET_GALAXY flag (bestPrimtarget = 64), and ones also with other flags. It is found that for the second class Main galaxies, the early-type proportion monotonously increases with increasing luminosity nearly in the whole luminosity region. But for the first class Main galaxies, the early-type proportion increases with increasing luminosity only within a certain luminosity region (−22.2 < M _r  < −19.8). In the high luminosity region (M _r  < −22.2), the early-type proportion of the first class Main galaxies even decreases dramatically with increasing luminosity. We also analyze the correlation between morphologies and luminosity of galaxies around the peak of the redshift distribution ( 0.07 ≤ z ≤ 0.08 ). In such a narrow redshift region, we still observe strong correlation between morphologies and luminosity, which shows that this correlation is fundamental.     

非饱和黄土渗透性规律的土柱试验研究

黄土边坡的变形破坏一般与地表水入渗导致的地下水位上升有关。然而,现场观测发现黄土地区地表水入渗深度有限,降雨的湿润峰一般在2m以内。自湿润峰以下至地下水位之间很长一段的含水率是不变的,那么地表水是如何补给地下水的,一直存在争议。为此,本文利用甘肃正宁县地区的Q3黄土重塑样进行非饱和渗透特性的土柱试验。在一个4m高的玻璃桶内制备土样,土柱上按一定间距插入水分计探头,在顶部按每天1000mL水量均匀渗入水,测得给定时间沿土柱的含水率剖面。结果发现,随着补给时间的延长,湿润峰下移,湿润峰经过的上半土柱含水率几乎不变,当湿润峰到达土柱底部时,形成潜水位,这和现场观察的现象一致。这说明在地表活动带以下,饱和带以上,虽然土的含水率不变,但存在着稳定非饱和渗流,这是黄土地区地下水的唯一补给方式。     

大地电磁测深法在慈页1井定位中的应用

在灰岩发育地区进行钻探作业时经常会遇到溶洞,给钻探带来不小的风险.为了减小钻探风险,可以采用探测深度大、对溶洞识别能力强的大地电磁测深法进行溶洞探测,确定钻孔的有利位置.本文以慈页1井的钻孔定位研究为例,通过在井场开展大地电磁测深工作,查明井场下方可能有溶洞发育的区域,最终确定了孔位的有利位置,在实际钻进过程中并未遇到溶洞发育段,说明通过大地电磁测深法布置的孔位合理,保证了钻探的安全施工.