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1.
流沙是我国沙漠化主要成因之一。本文简要回顾了我国北方沙漠及受沙漠化影响的干旱半干旱地区为保护交通线路而采取的固沙措施和技术,包括工程措施、化学措施和生物措施,主要介绍了这些措施和技术的类型及特点,以及近60年间(1950–2010年)其在不同地区不同交通线路中的应用,包括包兰线、塔里木沙漠公路和青藏铁路沿线的防风固沙。工程措施,如建挡风墙和铺设沙障,在沙漠交通线的防风固沙中非常有效。化学措施因成本高和对环境可能造成的污染风险而应用并不普遍。生物措施比工程和化学措施成本更高,但因其效果好且防护持续时间长而得到推崇。在一些地方,几种措施组合的固沙效果更好。工程措施对沙面的固定以及有条件的地方用地下水或河水灌溉有助于旱生植物的早期定植。本文最后指出了固沙措施和技术的局限性以及未来研究方向。本文对解决蒙古高原受沙漠和沙漠化影响的干旱和半干旱地区与"一带一路"倡议相关的基础设施建设的生态环境问题具有重要意义。  相似文献   
2.
基于Open Stack的开源标准体系,结合中国地震台网中心和中国地震局第二监测中心的云基础设施现状,设计两级云管理架构,以异构云管理平台作为综合管理平台,纳管区域云管理平台,以统一门户的方式对地震行业云计算资源进行统一管理;通过容器化部署异构云管理平台,初步实现对地震行业云计算资源的统一监控和运行管理。  相似文献   
3.
Throat aurora was defined based on the ground observations near local noon and has been suggested to be the ground signature of an indentation on the subsolar magnetopause. A global view of the auroral oval with throat aurora will be critical for inferring global processes at the magnetopause, but it has never been achieved. Using imaging spectrograph observations from Defense Meteorological Satellite Program satellites, for the first time, here we show typical throat auroras in a global view and reveal some important observational facts as follows.(1) The throat auroras can be as long as ~8 degrees in latitudinal direction,which is hardly to be fully seen in the ground-based camera.(2) The plasma flows and field aligned currents associated with throat aurora show consistences with previous radar observations, which have been suggested to be the observational evidence of magnetopause reconnection.(3) Most importantly, we confirmed that the electron and ion precipitations associated with throat aurora are always spatially separated, i.e., electrons in the east and ions in the west. The observational results not only establish a new picture of the aurora oval near local noon, but also provide important support to a conceptual model of throat aurora.  相似文献   
4.
The 2018 typhoon season in the western North Pacific(WNP) was highly active, with 26 named tropical cyclones(TCs) from June to November, which exceeded the climatological mean(22) and was the second busiest season over the past twenty years. More TCs formed in the eastern region of the WNP and the northern region of the South China Sea(SCS). More TCs took the northeast quadrant in the WNP, recurving from northwestward to northward and causing heavy damages in China's Mainland(69.73 billion yuan) in 2018. Multiscale climate variability is conducive to an active season via an enhanced monsoon trough and a weakened subtropical high in the WNP. The large-scale backgrounds in 2018 showed a favorable environment for TCs established by a developing central Pacific(CP) El Ni?o and positive Pacific meridional mode(PMM)episode on interannual timescales. The tropical central Pacific(TCP) SST forcing exhibits primary control on TCs in the WNP and large-scale circulations, which are insensitive to the PMM. During CP El Ni?o years, anomalous convection associated with the TCP warming leads to significantly increased anomalous cyclonic circulation in the WNP because of a Gill-type Rossby wave response. As a result, the weakened subtropical high and enhanced monsoon trough shift eastward and northward, which favor TC genesis and development. Although such increased TC activity in 2018 might be slightly suppressed by interdecadal climate variability, it was mostly attributed to the favorable interannual background. In addition, high-frequency climate signals,such as intraseasonal oscillations(ISOs) and synoptic-scale disturbances(SSDs), interacted with the enhanced monsoon trough and strongly modulated regional TC genesis and development in 2018.  相似文献   
5.
Carbon-enhanced metal-poor (CEMP) stars are considered to be related to the first generation of stars, and responsible for the chemical evolution of the early Galaxy. More than half of them are in binaries, and could be explained by the binary evolution, but the formation channel of them is still not fully understood. Among the hundreds of CEMP stars, there are nine CEMP RR Lyrae stars identified, and at least seven of which are very likely not binaries. The usual binary star evolution channel is difficult to produce such a single star, particularly that of carbon enrichment. One way in which such a single star might be produced is the merger of a helium white dwarf with a Hertzsprung gap (HG) star. We use a stellar evolution program to calculate the models of the merger remnants, and find that the models can reproduce the observed distribution of these CEMP single RR Lyrae stars in terms of surface temperature, gravity, and carbon abundance. Hence, it is extremely possible that the helium white dwarf and HG star merger model is one of the formation channels of the metal-poor carbon-rich RR Lyrae stars.  相似文献   
6.
基于正交匹配追踪的声层析方法   总被引:2,自引:0,他引:2  
声速剖面的变化会对声传播产生较大的影响,经验正交函数模型经常用来实现对声速剖面数据的简化描述。然而在内波、湍流等海水不均匀性存在时,这种正则化操作会造成声速重构精度的大幅降低。本文利用字典学习生成声速剖面的非正交原子,在稀疏编码时采用正交匹配追踪(OMP,Orthogonal Matching Pursuit)算法,更新字典则使用KSVD (Kernel Singular Value Decomposition)的字典更新算法。由于字典学习不需要强制使用正交条件,对于训练数据更加灵活,从而可以使用少数的原子组合达到更高的重构精度。利用一次浅海声学实验多次测量的声速剖面研究了海水声速剖面的经验正交函数表示和字典学习,研究表明:相比于正交函数表示,学习字典可以利用少数原子(甚至一个原子)更好的解释声速剖面扰动。字典学习可以提高声速剖面的稀疏性,从而提高声速剖面的反演精度。  相似文献   
7.
Active hydrogen maser is the main frequency standard for establishing and maintaining the time scale. It has the characteristics of high short-term stability and low phase noise. At present, it plays an increasingly important role in the international atomic time (TAI) and various local time scales. Firstly, in combination with the internal state parameters of an active hydrogen maser, the correlation between the internal state parameters and the comparison data of a hydrogen maser is analyzed, and a method for the performance monitoring of a hydrogen maser is proposed. Secondly, according to the characteristics of hydrogen maser performance, a method for evaluating the performance of a hydrogen maser is given. The hydrogen maser performance includes mainly two aspects, namely the frequency stability and predictability. The performances of two types of active hydrogen masers (CH1-75 and MHM-2010) are evaluated by this method. The correlation analysis of the atomic clock state parameters and comparison data shows that the state parameter monitoring can effectively predict the variation of the hydrogen maser performance. The evaluation results of atomic clock frequency stability and predictability show that the atomic clock with a higher medium-and-long term frequency stability has a better predictability. There are two methods for the predictability evaluation, one is based on the data published by BIPM (Bureau International des Poids et Measures), and another one is based on the quadratic model. Both methods are consistent with the weights published by BIPM. Therefore, the two methods can be used as a quantitative method to evaluate the predictability of a hydrogen maser.  相似文献   
8.
地层横波波速测量以及各向异性评价是目前随钻声波测井应用及方法研究的难题之一.针对这些问题,本文试图从钻铤上的偏心点声源在各向异性地层中的响应出发,寻求和探讨解决方案.我们基于三维有限差分模拟的随钻测井信号,研究了偏心点声源在水平横向各向同性(HTI)慢速地层井孔中激发声波传播规律,研究结果表明:在HTI地层中偏心点声源能够同时激发出快、慢两种波形,并且此两种波形中主要分别包含快、慢弯曲波,由于与钻铤波的耦合作用,其速度总是分别小于地层快、慢横波波速,所以无法直接用于地层横波波速的测量.但根据进一步的灵敏度分析可知当在3kHz以上时,它们的相速度分别对地层参数水平和垂直剪切模量(c66和c44)最为敏感.基于此特性,本文提出一种基于解析近似解的最小二乘拟合法,能够通过快、慢波频散曲线反演地层横波波速,所测值误差小于3%,并且具有很好的容错率和稳定性;进而由横波速度反演值评价地层各向异性大小.最后,地层快横波偏振方位可以利用垂直于偏心声源方向的偶极采集的信号能量变化曲线来获取.  相似文献   
9.
Chen  Haitao  Li  Jinhua  Wu  Long-Fei  Zhang  Wei-Jia 《中国海洋湖沼学报》2021,39(6):2015-2026
Journal of Oceanology and Limnology - Magnetotactic bacteria (MTB) are morphologically and phylogenetically diverse prokaryotes commonly able to produce magnetic nanocrystals within intracellular...  相似文献   
10.
Zhou  Kan  Liu  Baoyin  Fan  Jie 《地理学报(英文版)》2020,30(8):1363-1381
Journal of Geographical Sciences - The border areas of the Tibetan Plateau and the neighboring mountainous areas have a high incidence of earthquakes with a magnitude greater than Ms 5.0, as well...  相似文献   
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