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基于ISM的互联网金融信任机制形成的影响因素分析
互联网金融 信任机制 网络道德水平 平台声誉
2018/11/16
互联网金融的创新发展引起了各界的关注,在面对诸多风险和不确定性因素时,互联网金融信任机制的形成对互联网金融的运行起着关键作用。从资金持有方维度、资金需求方维度、交易维度和制度维度提取10个影响互联网金融信任机制形成的因素,基于解释结构模型的研究方法构建影响因素的关系结构模型,结果发现:资金持有方的信任倾向和风险感知能力是影响信任机制形成的直接因素,而互联网整体的网络道德水平对互联网金融信任机制的形...
随着BOT融资形式在我国基础设施建设中的广泛应用,对其风险的评估也变得愈加重要。本文以BOT项目融资风险为分析对象,对政治、法律、金融、建设、运营、移交等方面形成的风险进行研究,构建风险影响因素指标体系,运用ISM将影响因素分层,并构建多层阶梯解释结构模型。依据ISM模型,用ANP方法确定风险影响因素的权重,得出影响风险评价的主要因素。研究结果表明:分析结果符合实际情况,此种分析模式可为以后的BO...
Evidence for Correlated Titanium and Deuterium Depletion in the Galactic ISM
abundances abundances
2014/12/24
Current measurements indicate that the deuterium abundance in diffuse interstellar gas varies spatially by a factor of ~4 among sightlines extending beyond the Local Bubble. One plausible explanation ...
The quantity of dust in a spiral disk can be estimated using the dust's typical emission or the extinction of a known source. In this paper we compare two techniques, one based on emission and one on ...
A Systematic Study of the Stellar Populations and ISM in Galaxies out to the Virgo Cluster
stellar archeology star formation
2014/12/22
We present a compelling case for a systematic and comprehensive study of the resolved and unresolved stellar populations, ISM, and immediate environments of galaxies throughout the local volume, defin...
A Systematic Study of the Stellar Populations and ISM in Galaxies out to the Virgo Cluster: near field cosmology within a representative slice of the local universe
feedback near-fi eld cosmology
2014/12/22
We present a compelling case for a systematic and comprehensive study of the resolved and unresolved stellar populations, ISM, and immediate environments of galaxies throughout the local volume, defin...
基于ISM的火力发电企业成本控制
ISM 火力发电企业 成本控制 费用
2015/7/31
本文利用KJ法对火力发电企业的成本问题进行探讨,从企业自身的角度探寻影响成本控制的主要因素。进而建立成本控制解释结构模型,利用ISM解释影响成本控制的直接因素和深层因素,并提出控制火力发电企业成本的建议。
基于ISM的装甲车辆全寿命周期风险分析模型
装甲车辆 全寿命风险分析 ISM 解释层次分析法
2015/10/16
针对装甲车辆自身特点,对其全寿命周期风险识别与评估进行了深入研究。首先通过霍尔三维结构原理探讨了装甲车辆全寿命周期的主要风险类别;其次,运用解释结构模型(ISM)对各风险源之间的关系进行探索;最后,针对解释结构模型对风险总体水平评价的不足,提出了一种改进方法——解释层次分析法,并运用它对装甲车辆全寿命风险作实证研究。
Interpreting Anarch ism and Anti-Colonial Nationalism Contrapuntall y
Anarch ism Anti-Colonial Nationalism Contrapuntall y
2014/2/17
Interpreting Anarch ism and Anti-Colonial Nationalism Contrapuntall y。
基于ISM模型的影响中韩FTA缔结因素分析
中韩FTA ISM模型 影响因素 对策
2013/8/8
本文通过构建ISM模型对影响中韩FTA缔结的因素进行分析,得出不平衡的中韩对外直接投资关系是影响两国缔结FTA的最大因素;另外,贸易不平衡与摩擦、FTA战略动机的差异、对产业“空洞化”的担心也是影响两国缔结FTA的深层次因素。最后提出缔结中韩FTA的政策建议,如不断扩大中国对韩国的对外直接投资、缩减贸易逆差、发展产业内贸易等政策建议。
Classifying structures in the ISM with Support Vector Machines: the G16.05-0.57 supernova remnant
Classifying structures Support Vector Machines supernova remnant
2011/10/20
We apply Support Vector Machines -- a machine learning algorithm -- to the task of classifying structures in the Interstellar Medium. As a case study, we present a position-position velocity data cube...
基于ISM结构模型的成都市政府重大投资项目决策风险研究
结构模型解析法 政府重大投资项目 决策风险
2012/9/11
借助结构模型解析法,针对成都市政府重大投资项目决策涉及到的各风险因素来源主体,可能导致的各种风险因素,建立了成都市政府重大投资项目决策风险因素来源体递阶结构图。并对不同来源体、不同层次间的相互作用与影响进行了较为全面的分析,继而提出了加强政府投资决策管理,回避决策风险的建议。
A Detailed Study of the Molecular and Atomic Gas Toward the γ-ray SNR RX J1713.7-3946: Spatial TeV γ-ray and ISM Gas Correspondence
McClure-Griffi ths G. Rowel T. Inoue S. Inutsuka A. Kawamura
2011/9/27
RX J1713.7-3946 is the most remarkable TeV {\gamma}-ray SNR which emits {\gamma}-rays in the highest energy range 10-100 TeV. We made a combined analysis of CO and HI in the SNR and derived the total ...
The Evolution of the Large-scale ISM: Bubbles, Superbubbles and Non-Equilibrium Ionization
the Large-scale ISM Bubbles Superbubbles
2011/1/11
The ISM, powered by SNe, is turbulent and permeated by a magnetic field (with a mean and a turbulent component). It constitutes a frothy medium that is mostly out of equilibrium and is ram pressure do...
ISM enrichment and local pollution in dwarf galaxies
Cosmology and Extragalactic Astrophysics (astro-ph.CO) Galaxy Astrophysics (astro-ph.GA)
2010/12/28
The fate of metals after they are released in starburst episodes is still unclear. What phases of the interstellar medium are involved, in which timescales?