基于飞机观测资料的石家庄秋季对流层CH4垂直分布特征

为研究石家庄秋季对流层内CH₄垂直分布特征,2018年9月使用“空中国王350”飞机搭载Picarro温室气体在线观测仪和气象要素观测设备,对石家庄上空（600—5500 m）CH₄浓度进行探测。探测期间共飞行7架次,取得7条CH₄浓度廓线数据。结果表明: 石家庄上空近地面层（1000 m以下）CH₄平均浓度与同时间段区域背景站上甸子站CH₄浓度呈显著正相关（r=0.81,P < 0.03）。探测到的CH₄浓度最小值为1898×10^-9摩尔分数,最大值为2219×10^-9摩尔分数,平均浓度为1981×10^-9摩尔分数。观测得到的7条廓线均有较好的一致性,2000 m以上,浓度均随高度呈先增大后减小的趋势。利用后向轨迹模式（HYSPLIT）对探测时段内石家庄上空不同高度层主要气流传输路径进行统计分析表明,600 m高度输送路径较短,CH₄浓度受本地排放影响较大; 3000 m受输送作用影响较大,偏西和西南路径可能将较高CH₄浓度气团输送至石家庄上空; 5000 m气团传输对CH₄浓度影响较小,浓度相对较稳定,对传输路径的变化不敏感。     

“SZ-4”飞船高度计天线指向角反演方法

利用2003年2月7到8日“SZ-4”高度计的波形数据,经过波形数据预处理(波形为1 s的平均、去除热噪声和波形归一化)后,对海面回波波形后沿进行拟合,计算出了高度计天线的指向角,结果表明,“SZ-4”飞船高度计天线的指向角几乎全部在0.024°以内,天线指向在计算时间内比较稳定.     

添加剂对KAlSi_3O_8-CaSO_4-CaCO_3体系反应表观活化能的影响

首先测定了KAlSi3O8-CaSO4-CaCO3体系在不同焙烧条件下钾长石转化成可溶性氧化钾的转化率,进而通过模拟计算表明:KAlSi3O8-CaSO4-CaCO3体系的固相扩散动力学过程符合金斯特林格动力学方程,反应表观活化能Ea为128.92kJ/mol。并着重考察了4种添加剂Na2SO4、Na2SO3、NaCl和NaF对KAlSi3O8-CaSO4-CaCO3体系的影响,结果表明:向体系中分别加入占反应物总质量3%的Na2SO4、Na2SO3、NaCl和1%的NaF后,体系的反应表观活化能Ea从原来的128.92kJ/mol依次下降至87.15、98.71、117.38和126.14kJ/mol,这表明4种添加剂中Na2SO4的效果最好,它能较大程度上降低反应表观活化能,从而降低反应温度和提高固相反应速率。     

Deciphering the depositional environment of the laminated Crato fossil beds (Early Cretaceous,Araripe Basin,North‐eastern Brazil)

The laminated limestones of the Early Cretaceous Crato Formation of the Araripe Basin (North‐eastern Brazil) are world‐famous for their exceptionally well‐preserved and taxonomically diverse fossil fauna and flora. Whereas the fossil biota has received considerable attention, only a few studies have focused on the sedimentary characteristics and palaeoenvironmental conditions which prevailed during formation of the Crato Fossil Lagerstätte. The Nova Olinda Member represents the lowermost and thickest unit (up to 10 m) of the Crato Formation and is characterized by a pronounced rhythmically bedded, pale to dark lamination. To obtain information on palaeoenvironmental conditions, sample slabs derived from three local stratigraphic sections within the Araripe Basin were studied using high‐resolution multiproxy techniques including detailed logging, petrography, μ‐XRF scanning and stable isotope geochemistry. Integration of lithological and petrographic evidence indicates that the bulk of the Nova Olinda limestone formed via authigenic precipitation of calcite from within the upper water column, most probably induced and/or mediated by phytoplankton and picoplankton activity. A significant contribution from a benthonic, carbonate‐secreting microbial mat community is not supported by these results. Deposition took place under anoxic and, at least during certain episodes, hypersaline bottom water conditions, as evidenced by the virtually undisturbed lamination pattern, the absence of a benthonic fauna and by the occurrence of halite pseudomorphs. Input of allochthonous, catchment‐derived siliciclastics to the basin during times of laminite formation was strongly reduced. The δ¹⁸O values of authigenic carbonate precipitates (between ?7·1 and ?5·1‰) point to a ¹⁸O‐poor meteoric water source and support a continental freshwater setting for the Nova Olinda Member. The δ¹³C values, which are comparatively rich in ¹³C (between ?0·1 and +1·9‰), are interpreted to reflect reduced throughflow of water in a restricted basin, promoting equilibration with atmospheric CO₂, probably in concert with stagnant conditions and low input of soil‐derived carbon. Integration of lithological and isotopic evidence indicates a shift from closed to semi‐closed conditions towards a more open lake system during the onset of laminite deposition in the Crato Formation.     

4D architecture and tectonic evolution of the Laverton region,eastern Yilgarn Craton,Western Australia

The Laverton region, located in the eastern Yilgarn Craton (EYC) Western Australia, is second only to the Kalgoorlie region for gold endowment. The integration of high-density, potential-field data, regional- and camp-scale seismic reflection data, regional- and mine-scale structural analysis, and geochronologically-constrained stratigraphy, provided new insights into the 4D architecture and tectonic evolution of Laverton region.     

基于ARM7的嵌入式三维电阻率采集子站的设计研究

提出了一种基于ARM7的嵌入式三维电阻率采集子站设计方法,采用24位A/D转换器（ADS1258）和ARM7微处理器（LPC2378）,使三维电阻率法数据采集系统具有体积小、功耗低、成本低、精度高等特点,同时实现μC/OSⅡ操作系统在ARM的移植,为数据采集的实时性提供可能。     

充气欠平衡钻井液技术在DP4井水平段的应用

DP4井是中石化华北分公司在鄂尔多斯盆地大牛地气田布置的一口充气欠平衡水平井,该井目的层为盒1段,地层压系数较低,压力系数范围0．83—0．99（平均0．93）,为了有效保护气层,DP4井水平段全过程采用了充气欠平衡钻井工艺技术。欠平衡钻井工艺采用充气钻井液技术,通过该工艺在DP4井的实施,在盒1气层保护上取得较大成功。主要介绍了充气欠平衡钻井液技术的技术工艺、实施过程和现场实施情况,并对充气欠平衡钻井液技术在该井实施效果进行了分析评价。     

勘察设计企业并购模式的选择

随着我国社会主义市场经济体制改革的不断深化,加入WTO后与国际市场融入度的不断加强,企业生存与发展的环境日益呈现出市场一体化、需求多元化、竞争激烈化的特征,为了拓展企业的业务范围、扩大企业规模以及提高市场的竞争实力以应对日益激烈的市场竞争,勘察设计企业面对严峻的市场和竞争环境,结合企业自身的资源、环境和并购目的选择合适的并购模式,通过借助并购等资本运营手段,将企业做大做强,增强其综合实力,有效参与全球竞争。     

Spatial and seasonal variation of major ions in Himalayan snow and ice: A source consideration

The spatial and temporal variation of major ions (Ca²⁺, Mg²⁺, Na⁺, K⁺, , , and Cl⁻) in Himalayan snow and ice is investigated by using two snow pits from the East Rongbuk glacier (28°01′N, 86°58′E, 6500 m a.s.l.), one snow pit from the Nangpai Gosum glacier (28°03′N, 86°39′E, 5700 m a.s.l.), one snow pit from the Gyabrag glacier (28°11′N, 86°38′E, 6303 m a.s.l.), and three ice cores from the Sentik (35°59′N, 75°58′E, 4908 m a.s.l.), Dasuopu (28°33′N, 85°44′E, 7000 m a.s.l.), and East Rongbuk (27°59′N, 86°55′E, 6450 m a.s.l.) glaciers, respectively. In general, the major ions show a significant seasonal variation, with high concentrations during the non-monsoon (pre-monsoon and post-monsoon) season and relatively low concentrations during the monsoon season. Monsoon precipitation with high local/regional dust loading related to summer circulation is possibly responsible for the high concentrations occurring sporadically during the monsoon season. The crest of the Himalayas is an effective barrier to the spatial distribution of Na⁺, Cl⁻ and concentrations, but not to the major ions associated with dust influx (e.g. Ca²⁺ and Mg²⁺). Atmospheric backward trajectories from the HYSPLIT_4 model used in identifying chemical species sourcing suggest that the major ions in the Himalayan snow and ice come mainly from the Thar Desert located in the North India, as well as West Asia, or even the distant Sahara Desert in the North Africa during the winter and spring seasons. This is different from the conventionally assumed arid and semi-arid regions of the central Asia. Factors, such as different vapor sources due to atmospheric circulation patterns and geographical features (e.g. altitude, topography), may contribute to the differences in major ionic concentrations between the western and eastern Himalayas.