GM4型磁通门磁力仪性能检验方法

目前,磁通门磁力仪广泛应用于观测地球磁场相对变化的仪器。相对于应用,仪器的性能测试不为人们所熟悉。本文针对GM4型磁通门磁力仪的噪声特性,频率特性,线性度,温度特性等关键性能指标的测试依据、测试方法及流程给予详细的阐述。     

柴达木盆地东部地区石炭系泥页岩生烃条件及选区

柴达木盆地石炭系露头、钻井资料均揭示,其为海相沉积烃源岩,且石炭系泥页岩气展现出良好的勘探前景。对柴达木盆地东部石炭系泥页岩沉积环境、有机质丰度、类型和演化程度进行综合评价,利用野外露头、探井、地震、非震等资料证实了石炭系的残留及分布。研究认为,柴东地区石炭系泥页岩主要集中在上石炭统滨岸潮坪沉积的克鲁克组,发育炭质泥页岩、暗色泥岩2种烃源岩,有机碳均值为3.08%,有机质类型为Ⅱ-Ⅲ型,处于成熟-高成熟演化阶段,73%的样品达到中等-好烃源岩。平面上主要分布于尕丘、欧南、霍布逊和德令哈凹陷,分隔性较强,具有多个厚度中心,其中以欧南凹陷石灰沟地区和霍布逊凹陷落实程度高、资源潜力大,是泥页岩气最有利的发育区。     

初值及物理过程对\

利用国防科技大学全球中期数值天气预报模式（YinHe Global Spetral model,YHGS）产品驱动WRF对2018年7月4日华中地区暴雨过程进行模拟,并与ERA-interim资料作初始场模拟结果对比,评估YHGS模式产品在此次暴雨过程预报中的应用能力。结果表明：（1）WRF-YHGS对2018年7月4日华中地区暴雨过程有一定的预报能力,其模拟的大尺度环流形势、水汽收支量变化趋势与WRF-ERA有着很好的一致性,YHGS模式产品驱动中尺度数值预报是可行的。（2）WRF-YHGS模拟效果较WRF-ERA差,但大雨量级WRF-ERA湿偏差较大,两组试验各物理量模拟结果存在一定差距,且随着积分时间的增加差异逐渐增大。（3）WRF-YHGS、WRF-ERA模拟结果的差异主要来自YHGS与ERA初始场中差异较大的次天气尺度运动和YHGS全球模式预报场误差两个方面。

     

地球磁场对太阳风的加载响应与地震

地磁预报地震的方法越来越多,本文应用加卸载响应比方法,分析山西地区2009—2016年观测的加卸载响应比与山西地区4.0级地震之间的对应关系,初步给出适用于山西地区震例特征的磁异常判别指标。     

Climatic and geographic factors affect ecosystem multifunctionality through biodiversity in the Tibetan alpine grasslands

Ecosystem multifunctionality(EMF), the simultaneous provision of multiple ecosystem functions, is often affected by biodiversity and environmental factors. We know little about how the interactions between biodiversity and environmental factors affect EMF. In this case study, a structural equation model was used to clarify climatic and geographic pathways that affect EMF by varying biodiversity in the Tibetan alpine grasslands. In addition to services related to carbon, nitrogen, and water cycling, forage supply, which is related to plantproductivity and palatability, was included in the EMF index. The results showed that 72% of the variation in EMF could be explained by biodiversity and other environmental factors. The ratio of palatable richness to all species richness explained 8.3% of the EMF variation. We found that air temperature, elevation, and latitude all affected EMF, but in different ways. Air temperature and elevation impacted the aboveground parts of the ecosystem, which included plant height, aboveground biomass, richness of palatable species, and ratio of palatable richness to all species richness. Latitude affected EMF by varying both aboveground and belowground parts of the ecosystem, which included palatable speciesrichness and belowground biomass. Our results indicated that there are still uncertainties in the biodiversity–EMF relationships related to the variable components of EMF, and climatic and geographic factors. Clarification of pathways that affect EMF using structural equation modeling techniques could elucidate the mechanisms by which environmental changes affect EMF.     

Dark energy model in anisotropic Bianchi type-III space-time with variable EoS parameter

A new dark energy model in anisotropic Bianchi type-III space-time with variable equation of state (EoS) parameter has been investigated in the present paper. To get the deterministic model, we consider that the expansion θ in the model is proportional to the eigen value s² ₂\sigma^{2}_{~2} of the shear tensor s^j _i\sigma^{j}_{~i}. The EoS parameter ω is found to be time dependent and its existing range for this model is in good agreement with the recent observations of SNe Ia data (Knop et al. in Astrophys. J. 598:102, 2003) and SNe Ia data with CMBR anisotropy and galaxy clustering statistics (Tegmark et al. in Astrophys. J. 606:702, 2004). It has been suggested that the dark energy that explains the observed accelerating expansion of the universe may arise due to the contribution to the vacuum energy of the EoS in a time dependent background. Some physical aspects of dark energy model are also discussed.     

外部利润、产权界定与土地资源优化配置——成都市农村土地股份合作制改革的制度经济学解析

以"外部利润——产权界定——资源优化配置"为研究主线,对成都市农村土地股份合作制改革进行了制度经济学解析。研究发现,制度创新空间的形成、土地的增值收益、土地规模利用效应和土地集约利用效应构成了成都市农村土地股份合作制改革的外部利润。成都市农村土地股份合作制改革,一方面可以提高土地规模和集约利用效应,促进土地资源优化配置;另一方面可以明晰集体土地产权主体,健全基层组织治理机制。要采取诸如放松法律限制、加强理论研究、规范机制建设等措施,从而推动土地股份合作制的生成和发展。     

HITRAN数据库对卫星1.6 μm通道CO2辐射传输特性计算的影响

卫星遥感器中的CO21.6μm弱吸收带通道测量信号可以反映CO2的近地层浓度分布,是温室气体卫星反演的重要通道之一。HITRAN数据库是建立卫星遥感CO2浓度算法依赖的重要分子光谱参数数据库,目前已经更新到了2012版,不同版本中大气分子谱线参数存在差异。本文利用逐线积分模式LBLRTM,研究了最近3个版本HITRAN数据库(04、08、12版)在CO2的弱吸收带通道上大气光学厚度、透过率的差异,发现04版计算的气体光学厚度普遍偏高,可对CO2造成约38 ppm的低估;08版本得到的气体光学厚度与12版本接近,反演相差2 ppm以内。在此基础上,分析了不同HITRAN数据库对整层CO2变化和近地层CO2变化的敏感性,结果表明:04版对整层和近地面大气的变化敏感性最强,并且放大了近地层信号;08版与12版对整层或近地层CO2的敏感度接近,两者经过卷积后得到的信号无差异。     

高光谱数据在数据库中的高效存储技术研究

通过分析高光谱数据的特点 ,结合数据库系统开发实践 ,提出了高光谱数据集 ,包括图像、光谱、属性等 ,在关系数据库中的存储规范。结合ORACLE数据平台 ,提出了 3种高光谱数据的存储模式 ,并结合应用实例进行对比 ,分析了各自的优缺点以及适用条件。