GAIM电离层同化方法进展

电离层是复杂的空间层结,其变化受太阳活动强度、地球磁场等因素影响。随着空间技术发展的需求,电离层天气变化成为目前空间天气预报最重要的内容之一。最近10年,人们利用卫星在电离层观测方面取得了重大进展,尤其引人注意的是:无线电掩星观测技术正走向应用的新阶段,加上已经建立的全球大量的地基GPS观测网,它们不仅为电离层动力学模式研究提供了丰富的电离层资料,而且为电离层预报提供了很好基础。因此,电离层天气预报成为当前重要的、前瞻性的研究方向,电离层资料同化是电离层预报最重要的研究内容之一。该文系统介绍这方面国际动态,重点是美国的USC/JPL和犹他州大学开展全球电离层同化模型研究、全球电离层同化研究的进展,以及在电离层天气预报中应用的初步成果。     

On the ultracompact nature of 4U 1822−000

We report the discovery of a periodic modulation in the optical lightcurve of the candidate ultracompact X-ray binary 4U 1822−000. Using time-resolved optical photometry taken with the William Herschel Telescope we find evidence for a sinusoidal modulation with a semi-amplitude of 8 per cent and a period of 191 min, which is most likely close to the true orbital period of the binary. Using the van Paradijs & McClintock relation for the absolute magnitude and the distance modulus allowing for interstellar reddening, we estimate the distance to 4U 1822−000 to be 6.3 kpc. The long orbital period casts severe doubts on the ultracompact nature of 4U 1822−000.     

鄂尔多斯盆地奥陶系马家沟组四段构造- 岩相古地理新认识及勘探意义

米探1井取得天然气勘探突破表明鄂尔多斯盆地奥陶系马家沟组四段具有巨大勘探潜力,然而,对盆地奥陶纪马四期古构造格局和岩相古地理研究还存在争议,制约了下步天然气勘探进程。为此,基于地震、野外露头、钻井、岩芯、微观薄片和测井等基础资料,对马家沟组四段构造- 岩相古地理开展了系统研究,确定了盆地奥陶纪马四期古构造格局,并恢复出马家沟组四段岩相古地理,预测了有利勘探区。研究结果表明：① 鄂尔多斯盆地奥陶纪马四期发育“两陆三隆四坳”的古构造格局,其中两陆为伊盟古陆和阿拉善古陆,三隆分别为中央古隆起、中条古隆起和神木- 志丹低隆起,四坳为西南边缘坳陷、桃利庙坳陷、府谷坳陷和柳林坳陷;② 马四期为碳酸盐岩内缓坡和中缓坡沉积,其中内缓坡又发育白云岩坪、含云膏坪、微生物丘、灰泥丘、砂屑滩、丘滩间海和灰质潟湖等7类微相;③ 古构造格局控制马家沟组四段沉积分异,微生物丘、灰泥丘和砂屑滩等3类有利储集相主要沿中央古隆起和神木- 志丹低隆起等古地貌高部位分布。因此认为,神木—靖边地区是有利储层发育区,且处于岩性相变带,生储盖配置关系好,具有良好的成藏条件,是天然气勘探的有利靶向区。     

The Effects of Land Cover Change on Regional Climate over the Eastern Part of Northwest China

A regional climate model(Reg CM4) is employed to investigate the impacts of land use/cover change(LUCC) on the climate over the eastern part of Northwest China(ENW) in the periods of 2001 and 2011. The results indicated that the LUCC in ENW, which was characterized by desert retreat, reforestation, and farmland expansion, led to significant local changes in surface air temperature(within ~0.3°C) and slight regional changes in precipitation(within ~15%) in summer. In the desert retreat area, the net absorbed shortwave radiation had a greater influence than evaporative cooling, leading to increases in the daily mean and maximum temperature. Besides, the daily mean and maximum temperatures increased in the reforestation area but decreased in the farmland expansion area. As surface albedo showed no significant change in these regions, the temperature increase in the reforestation area can be attributed to a decrease in evaporation, while the opposite effect appears to have been the case in the farmland expansion area.     

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。     

东营凹陷南斜坡沙四下亚段—孔店组原油地球化学特征及成因分类

东营凹陷南斜坡沙四下亚段—孔店组为一套紫红色或红色碎屑岩沉积,本身不具备生烃能力,因此对该层段原油成因的研究具有重要意义。在系统分析17个油砂和5个原油样品的生物标志物组合特征的基础上,将该区原油划分为4种成因类型。Ⅰ类原油分布于平方王地区和博兴洼陷,Pr/Ph0.8,Ph/nC180.6,伽马蜡烷含量极低,4-甲基甾烷、重排甾烷含量相对高,Ts/Tm、藿烷/甾烷值相对高,可能来源于一套淡水湖相环境下形成的、富含粘土矿物的泥岩。Ⅱ类原油分布于纯化—乐安构造带、陈官庄构造带,Pr/Ph0.6,Ph/nC182,伽马蜡烷含量高,4-甲基甾烷、重排甾烷含量低,Ts/Tm和藿烷/甾烷值低,可能与一套盐湖相泥岩或灰质泥岩有成因关系。Ⅲ类原油分布于青城北缓坡构造带,检测出25-降藿烷系列,伽马蜡烷含量介于Ⅰ类和Ⅱ类之间,可能为早期充注的Ⅱ类原油遭受生物降解后和晚期充注的Ⅰ类原油形成的混源油,且以晚期充注为主。Ⅳ类原油分布于王家岗地区孔店组,具有C29甾烷绝对优势和高含量的伽马蜡烷,推断为Ⅱ类原油和一种来源于浅湖—沼泽相的原油形成的混源油。     

Origin of Paleofluids in Dabashan Foreland Thrust Belt:Geochemical Evidence of 13C,18O and 87Sr/86Sr in Veins and Host Rocks

In the last ten years, with important discoveries from oil and gas exploration in the Dabashan foreland depression belt in the borderland between Shanxi and Sichuan provinces, the relationship between the formation and evolution of, and hydrocarbon accumulation in, this foreland thrust belt from the viewpoint of basin and oil and gas exploration has been studied. At the same time, there has been little research on the origin of fluids within the belt. Based on geochemical system analysis including Z values denoting salinity and research on δ13C, δ18O and 87Sr/86Sr isotopes in the host rocks and veins, the origin of paleofluids in the foreland thrust belt is considered. There are four principal kinds of paleofluid, including deep mantle-derived, sedimentary, mixed and meteoric. For the deep mantle-derived fluid, the δ13C is generally less than ?5.0‰PDB, δ18O less than -10.0‰PDB, Z value less than 110 and 87Sr/86Sr less than 0.70600; the sedimentary fluid is mainly marine carbonate-derived, with the δ13C generally more than ?2.0‰PDB, δ18O less than ?10.0‰PDB, Z value more than 120 and 87Sr/86Sr ranging from 0.70800 to 0.71000; the mixed fluid consists mainly of marine carbonate fluid (including possibly a little mantle-derived fluid or meteoric water), with the δ13C generally ranging from ?2.0‰ to ?8.0‰PDB, δ18O from ?10.0‰ to ?18.0‰ PDB, Z value from 105 to 120 and 87Sr/86Sr from 0.70800 to 0.71000; the atmospheric fluid consists mainly of meteoric water, with the δ13C generally ranging from 0.0‰ to ?10.0‰PDB, δ18O less than ?8.0‰PDB, Z value less than 110 and 87Sr/86Sr more than 0.71000. The Chengkou fault belt encompasses the most complex origins, including all four types of paleofluid; the Zhenba and Pingba fault belts and stable areas contain a simple paleofluid mainly of sedimentary type; the Jimingsi fault belt contains mainly sedimentary and mixed fluids, both consisting of sedimentary fluid and meteoric water. Jurassic rocks of the foreland depression belt contain mainly meteoric fluid.