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排序方式: 共有501条查询结果,搜索用时 15 毫秒
91.
选取内蒙古锡林郭勒盟与积雪有关的雪灾致灾指标, 以气温、 风速为气象条件孕灾环境指标, 坡度、 植被盖度为下垫面孕灾环境指标, 人口密度、 牧民纯收入、 人均GDP、 牲畜超载率等数据为承灾体脆弱性指标, 基于BP方法、 层次分析法、 建立了内蒙古锡林郭勒盟白灾综合风险评价体系, 并对其进行了风险评价与区划。为提高灾害评估的准确率, 白灾的灾害等级是以月为尺度进行评定, 选取的气象指标多数都是以月为尺度的指标。研究表明: 白灾与积雪因子高度相关, 是气候灾害, 积雪、 低温、 大风等气象因子长期作用的结果。对白灾尝试用BP神经网络法进行风险评估, 评估的灾害等级和实际灾害等级十分吻合, 用训练好的神经网络对各个旗县(1980 - 2015年)的白灾进行了风险评估, 评估效果理想。因此, 可以通过数值预报产品、 气候预测产品获取相关评价因子, 采用BP方法形成白灾风险预评估产品, 进而应用于雪灾风险评估业务中, 为相关部门提供决策依据。  相似文献   
92.
Long hydroclimate records are essential elements for the assessment and management of changing freshwater resources. These records are especially important in transboundary watersheds where international cooperation is required in the joint planning and management process of shared basins. Dendrochronological techniques were used to develop a multicentury record of April 1 snow water equivalent (SWE) for the Stikine River basin in northern British Columbia, Canada, from moisture‐sensitive white spruce (Picea glauca) tree rings. Explaining 43% of the instrumental SWE variability, to our knowledge, this research represents the first attempt to develop long‐term snowpack reconstructions in northern British Columbia. The results indicated that 15 extreme low April 1 SWE events occurred from 1789 to the beginning of the instrumental record in 1974. The reconstruction record also shows that the occurrence of hydrological extremes in the Stikine River basin is characterized by persistent below‐average periods in SWE consistent with phase shifts of the Pacific Decadal Oscillation (PDO). Spectral analyses indicate a very distinct in‐phase (positive) relationship between the multidecadal frequencies of variability (~40 years) extracted from the SWE tree‐ring reconstruction and other reconstructed winter and spring PDO indices. Comparison of the reconstructed SWE record with other tree‐ring‐derived PDO proxy records shows coherence at multidecadal frequencies of variability. The research has significant implications for regional watershed management by highlighting the hydrological response of the Stikine River basin to prior climate changes.  相似文献   
93.
李红梅  赵毅  马振锋  景丰 《探矿工程》2016,43(7):107-110
延长油田页岩气储层埋藏较深,地质条件复杂,页理构造发育,岩石物性极差,页岩易膨胀、分散。由于孔缝并存,页岩气储层比砂岩油藏具有更严重的微粒运移损害、储层应力敏感损害、水锁损害等特性。鉴于延长页岩储层太过致密,不能用常规方法进行渗透率测定。通过采用人造裂缝法测定钻井液对储层裂缝的污染程度来表征钻井液对储层的损害率。经人造裂缝法测定,延长油田现场使用的白油基钻井液体系对页岩气储层的污染渗透率恢复率达到91.060%,初步证实该体系具有良好的储层保护效果,可在延长油田进一步推广使用并验证。  相似文献   
94.
某超大型离心机基础埋置于复杂软土地基中,自振特性研究十分关键。分别建立离心机基础的等效土弹簧模型和实体地基模型,对比分析不同地基模拟方法下的模态分析结果;开展基于白噪声激励的动力时程分析,分析地基参振质量对自振特性的影响。结果表明:超大型离心机基础前两阶模态振型分别为水平横向和纵向的摆动;基于不同的地基模拟方法计算得到的振型结果一致,自振频率相差在10%以内;超大型离心机基础结构的前两阶地基参振质量分别为1.376倍和0.998倍的基础总质量,地基参振质量使得结构的振动响应幅值下降50%左右,频谱峰值频率减小约2 Hz。结论对大型埋置式动力机器基础的自振特性研究具有指导和参考意义。  相似文献   
95.
The Mount Lyell copper deposits are located in the middle Cambrian Mount Read volcanic belt of western Tasmania and consist of more than 24 separate copper–gold–silver orebodies. The dominant copper mineralisation style is disseminated pyrite–chalcopyrite subvertical pipes with subordinate chalcopyrite–bornite ± other copper phases, massive pyrite and base metal sulfides. A zonation in mineralisation style within the pipes is defined from chalcopyrite–magnetite at depth to chalcopyrite–pyrite at intermediate levels, to chalcopyrite–bornite at the shallowest level. Alteration is developed broadly symmetrically around the ore zones and zoned from quartz–chlorite–phengite ± biotite at depth to quartz–muscovite at intermediate levels, and a quartz–muscovite–pyrophyllite–zunyite assemblage at the shallowest levels. This is interpreted to be a result of a fluid that evolved from hot, reduced and neutral conditions at depth to cool, oxidised and acidic conditions at the shallowest level. The chalcopyrite–bornite deposits occur at the top of the hydrothermal system and are associated with intensely silicified rock and muscovite/pyrophyllite alteration. The close relationship of these deposits with the top of the pipes suggests they are part of a single mineralising event. Where the chalcopyrite–bornite deposits are juxtaposed with the Owen Group, rather than a simple chalcopyrite–bornite mineralogy, there are numerous other copper phases, which represent higher oxidation states and collectively suggest variable and fluctuating fluid conditions during deposition. It is proposed that these deposits are formed by an interaction of the reduced hydrothermal fluid with an oxidised fluid generated at very shallow levels within and during deposition of the Owen Group. Mineralisation within the middle Owen Group sandstones and clasts of altered rock within the middle and upper Owen Group sediments marks the end of the hydrothermal system. Around the entire edge of the Mt Lyell field, there is a variation in the white mica composition from proximal muscovite to distal phengite that represents the neutralisation of the hydrothermal fluid by fluid–wall rock interaction.  相似文献   
96.
通过1991 年6 月6 日一个复杂的太阳活动事件( 包括宽带射电运动Ⅳ型爆发、脉冲相伴生的白光耀斑、耀斑后环及其伴生的射电多重短周期( 约1 - 4 秒) 脉动现象等) 的分析,探讨了白光耀斑产生的射电辐射特征,根据太阳白光耀斑和射电运动Ⅳ型爆发产生的物理过程,着重讨论了射电运动Ⅳ型爆发、耀斑后环和短周期脉动现象,并认为它们可能是白光耀斑的对应物  相似文献   
97.
98.
安微淮南潘北煤矿–580 m水平探4孔与ES1C3上3-1孔在疏放太原组灰岩水时带有臭鸡蛋气味,且水流过程中伴有白色絮状漂浮物。通过采集水样,测试了出水孔水质及气体,分析了其形成原因。结果表明:气体为H2S,两出水孔的水质均具有低SO2–4、高HCO–3、弱碱性特征,白色絮状物为有机质和钙、镁物质的结合,该异常现象是脱硫酸与脱碳酸共同作用的结果。为及时处理异味对井下作业环境的影响,采用纳米二氧化钛–紫外光催化氧化法在室内对水进行硫化氢去除试验,其去除率为80%~90%,效果显著。  相似文献   
99.
Observations of a large population of millisecond pulsars (MSPs) show a wide divergence in the orbital periods (from approximately hours to a few months). In the standard view, low‐mass X‐ray binaries (LMXBs) are considered as progenitors for some MSPs during the recycling process. We present a systematic study that combines different types of compact objects in binaries such as cataclysmic variables (CVs), LMXBs, and MSPs. We plot them together in the so called Corbet diagram. Larger and different samples are needed to better constrain the result as a function of the environment and formations. A scale diagram showing the distribution of MSPs for different orbital periods and the aspects for their progenitors relying on accretion induced collapse (AIC) of white dwarfs in binaries. Thus massive CVs (M ≥ 1.1 M) can play a vital role on binary evolution, as well as of the physical processes involved in the formation and evolution of neutron stars and their magnetic fields, and could turn into binary MSPs with different scales of orbital periods; this effect can be explained by the AIC process. This scenario also suggests that some fraction of isolated MSPs in the Galactic disk could be formed through the same channel, forming the contribution of some CVs to the single‐degenerate progenitors of Type Ia supernova. Furthermore, we have refined the statistical distribution and evolution by using updated data. This implies that the significant studies of compact objects in binary systems can benefit from the Corbet diagram.Observations of a large population of millisecond pulsars (MSPs) show a wide divergence in the orbital periods (from approximately hours to a few months). In the standard view, low‐mass X‐ray binaries (LMXBs) are considered as progenitors for some MSPs during the recycling process. We present a systematic study that combines different types of compact objects in binaries such as cataclysmic variables (CVs), LMXBs, and MSPs. We plot them together in the so called Corbet diagram. Larger and different samples are needed to better constrain the result as a function of the environment and formations. A scale diagram showing the distribution of MSPs for different orbital periods and the aspects for their progenitors re  相似文献   
100.
Asteroseismology is a powerful tool used for detecting the inner structure of stars, which is also widely used to study white dwarfs. We discuss the asteroseismology of DAV stars. The period-to-period fitting method is discussed in detail, including its reliability in detecting the inner structure of DAV stars. If we assume that all observed modes of some DAV stars are the l = I cases, the errors associated with model fitting will be always large. If we assume that the observed modes are com- posed of I = 1 and 2 modes, the errors associated with model fitting in this case will be small. However, there will be modes identified as l = 2 that do not have ob- served quintuplets. G29-38 has been observed spectroscopically and photometrically for many years. Thompson et al. made 1 modes identifications in the star through the limb darkening effect. With 11 known I modes, we also study the asteroseismology of G29-38, which reduces the blind l fittings and is a fair choice. Unfortunately, our two best-fitting models are not in line with the previous atmospheric results. Based on factors like only a few observed modes, stability and identification of eigenmodes, identification of spherical degrees, construction of physical and realistic models and so on, detecting the inner structure of DAV stars by asteroseismology needs further development.  相似文献   
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