Projection of droughts and their socioeconomic exposures based on terrestrial water storage anomaly over China

Science China Earth Sciences - Global warming has altered the thermodynamic and dynamic environments of the climate system, thus affecting the energy budget and water cycle process of the...     

滇黔桂“金三角”地区晚三叠世地层碎屑物源示踪

三叠系是滇黔桂分布最广泛的岩系,赋存卡林型金矿等各种低温矿产。在前人研究基础上,运用LA-ICP-MS分析技术,对滇黔桂"金三角"地区的碎屑锆石进行了U-Pb测年。结果显示,大部分锆石具岩浆环带,Th/U值大于0.4,锆石U-Pb年龄集中在308~396 Ma、440~680 Ma、727~930 Ma、1004~1266 Ma、1400~1880 Ma、2360~2724 Ma六个区段。通过对比研究区及周围地块的碎屑锆石年龄分布特征,结合研究区岩相古地理、古海流及古流向,综合分析认为,研究区物源以越北古陆为主,同时湘粤桂构造山系和云开地区也可能提供了部分物源。该物源印证了古特提斯洋在印支期逐渐闭合,华南陆块与印支地块沿松马缝合带发生碰撞。     

融合先验物理信息的高精度智能可控源电磁反演算法

可控源电磁反演利用人工信号获取地下结构信息,为地质勘探和资源开发提供准确的数据支持。然而,传统电磁反演方法面临低分辨率的挑战,主要是由于简化处理和观测数据的限制,导致模型平滑、细节丢失,从而削弱了反演的准确性,影响了电磁勘探的效率。为了解决这一问题,本文提出将传统反演结果与响应数据同时作为深度网络的输入数据,为深度网络反演提供先验物理信息,并结合深度学习算法提升可控源电磁反演的计算效率。通过模型试验,对合成的电阻率模型分别进行了传统反演、智能反演以及融合先验物理信息的智能反演。结果表明,融合先验物理信息的智能反演能够更好地刻画异常体结构特征,有效提升反演效率,并且得到的电阻率参数更符合实际。最后,将该反演技术应用于金川铜镍矿床的可控源数据反演解释,取得了较为可靠的应用效果。     

Investigations into the thermal non-equilibrium of W UMa-type contact binaries

Traditionally, some physical details(e.g., magnetic braking, energy transfer, angular momentum loss, etc.) have to be taken into consideration during investigations into the evolution of contact binaries. However, the real evolutionary processes which usually contain several of these physical mechanisms are very complicated as a result of strong interaction between components. To avoid dealing with these factors, a linear relationship is applied to the temperatures of components. It is found that the higher the mass ratio(M_2/M_1) of a contact system, the weaker the deviation from thermal equilibrium.On this basis, a variation trend of fill-out factor(f) changing with mass ratio can be inferred, which is consistent with observations. Moreover, if we stick to this point of view, it should be natural that the number of semi-detached binaries in the predicted broken-contact phase of relaxation oscillations is less than the number in the contact phase.     

1–100 μm energy spectra and 2.3–4 μm spectrophotometry of MSC stars

The JHKL' photometry and 2.3–4 μm spectrophotometry of some M giants, S type stars and carbon stars are presented in this paper. It is found that in combination with IRAS data, the energy spectra in 1–100 μm of S type stars are intermediate between those of M giants and carbon stars, which are obviously different. The spectrophotometry in the near infrared shows that, besides carbon stars, which have HCN and C₂H₂ strong absorptions at 3.1 μm, some S type stars have the similar but weaker absorption in the same spectral region. However, no trace of any absorption at 3.1 μm can be seen in M giants. These results probably provide more evidence for the M-S-C sequence in the late stage of stellar evolution.     

Analysis on the interplanetary causes of the great magnetic storms in solar maximum (2000-2001)

In this paper, we analyze the interplanetary causes of eight great geomagnetic storms during the solar maximum (2000-2001). The result shows that the interplanetary causes were the intense southward magnetic field and the notable characteristic among the causal mechanism is compression. Six of eight great geomagnetic storms were associated with the compression of southward magnetic field, which can be classified into (1) the compression between ICMEs (2) the compression between ICMEs and interplanetary medium. It suggests that the compressed magnetic field would be more geoeffective. At the same time, we also find that half of all great storms were related to successive halo CMEs, most of which originated from the same active region. The interactions between successive halo CMEs usually can lead to greater geoeffectiveness by enhancing their southward field B_s interval either in the sheath region of the ejecta or within magnetic clouds (MCs). The types of them included: the compression between the fast speed transient flow and the slow speed background flow, the multiple MCs, besides shock compression. Further, the linear fit of the D_st versus gives the weights of and Δt as α=2.51 and β=0.75, respectively. This may suggest that the compression mechanism, with associated intense B_s, rather than duration, is the main factor in causing a great geomagnetic storm.     

新世纪测绘事业改革之我见

世纪交替之际 ,在信息社会和新经济条件下 ,我国测绘事业要发挥更大作用 ,必须抓住机遇 ,深化改革 ,以适应国家经济与社会发展的要求 ,仅就深化改革这一主题提出一些看法。     

水盐梯度下黄河三角洲湿地植被空间分异规律的定量分析

三角洲湿地植被的形成和分布同时受水深、土壤含盐量两个环境因子的作用。采用模糊数学排序方法分析了黄河三角洲湿地植被在水深、土壤含盐量两个环境梯度下的空间分异规律。结果表明,由TWINSPAN划分而得到的8个植被类型在模糊数学排序图中有各自的分布范围,界线明显。以穗状狐尾藻(Myriophyllum spica-tum)等水生植物为优势种的群落分布在排序图的左上部,为黄河三角洲湿地高水深、低盐分地区;以柽柳(Tam-arix chinensis)、翅碱蓬(Suaeda heteroptera)等典型盐生植物为优势种的群落分布在排序图的右下部,为黄河三角洲的低水深、高盐分地区;其他以芦苇(Phragmites australis)、荻(Triarrhena sacchariflora)、旱柳(Salix matsudana)等为优势种的群落分布在排序图的中部。利用Gini-Simpson指数,在模糊数学排序图中分析了植物物种多样性随水深、土壤含盐量梯度的空间变化,结果表明,高水深、低盐分和低水深、高盐分地区植物物种多样性均较低,而二者过渡区域植物物种多样性较高。     

方正断陷三维区沉积演化特征

应用层序地层学分层基础下的沉积学原理,依据各种数据,进行了各级层序单元的识别与划分,在本区识别出扇三角洲相、湖泊相和湖底扇相3类沉积相,进一步划分为8种沉积亚相和16种沉积微相;通过地震相研究及砂体的预测,进行了各层段微相的平面展布特征研究。结果表明研究区主要发育由方正断陷边缘和依汉通断裂向方正断陷中心推进的扇三角洲—湖泊沉积体系。