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71.
S. Zamfir J. W. Sulentic P. Marziani 《Monthly notices of the Royal Astronomical Society》2008,387(2):856-870
We search for a dichotomy/bimodality between radio-loud (RL) and radio-quiet (RQ) type 1 active galactic nuclei (AGN). We examine several samples of Slogan Digital Sky Survey (SDSS) quasi-stellar objects (QSOs) with high signal-to-noise ratio optical spectra and matching Faint Images of the Radio Sky at Twenty-cm/NRAO VLA Sky Survey (FIRST/NVSS) radio observations. We use the radio data to identify the weakest RL sources with a Fanaroff–Riley type II (FR II) structure to define a RL/RQ boundary which corresponds to log L 1.4 GHz = 31.6 erg s−1 Hz−1 . We measure the properties of broad-line Hβ and Fe ii emission to define the optical plane of a 4DE1 spectroscopic diagnostic space. The RL quasars occupy a much more restricted domain in this optical plane compared to the RQ sources, which a 2D Kolmogorov–Smirnov test finds to be highly significant. This tells us that the range of broad-line region kinematics and structure for RL sources is more restricted than for the RQ QSOs, which supports the notion of dichotomy. FR II and CD RL sources also show significant 4DE1 domain differences that likely reflect differences in line-of-sight orientation (inclined versus face-on, respectively) for these two classes. The possibility of a distinct radio-intermediate (RI) population between RQ and RL source is disfavoured because a 4DE1 diagnostic space comparison shows no difference between RI and RQ sources. We show that searches for dichotomy in radio versus bolometric luminosity diagrams will yield ambiguous results mainly because in a reasonably complete sample, the radio brightest RQ sources will be numerous enough to blur the gap between RQ and RL sources. Within resolution constraints of NVSS and FIRST, we find no FR I sources among the broad-line quasar population. 相似文献
72.
This paper investigates in detail the peak frequency of gyrosynchrotron radiation spectrum with self and gyroresonance absorption
for a model of nonuniform magnetic field. It is found that the peak frequency shifts from lower frequency to higher frequency
with increases in the low-energy cutoff, number density, input depth of energetic electrons, magnetic field strength and viewing
angle. When the number density and temperature of thermal electrons increase, the peak frequency also shifts to a slightly
higher frequency. However, the peak frequency is independent of the energy spectral index, high-energy cutoff of energetic
electrons and the height of the radio source’s upper boundary. It is also found for the first time that there is a good linear
correlation between the logarithms of the peak frequency and the low-energy cutoff, number density, input depth of energetic
electrons, magnetic field strength, and viewing angle, respectively. Their correlation coefficients are higher than 0.95 and
the standard errors are less than 0.06. 相似文献
73.
In the present work a statistical analysis of long-lived microbursts (MBs) in the decimetric wavelength range was performed
for the first time. Long-lived microbursts at decimetric wavelengths were observed with one-dimensional scans on the RATAN-600
radio telescope in intensity and circular polarization with a sensitivity of about 5 – 10 Jy. MBs have fluxes in the range
of 0.001 – 0.1 s.f.u. and polarization degrees of 10 – 100%, and the duration of individual bursts is about 1 – 2 s. Microbursts
and background sources exist for several days and appear at the sites of prolonged energy release. In this work MBs were compared
with noise storms (NSs) in the metric wavelength range. Our analysis shows with high confidence that MBs are manifestation
of NSs in the decimetric wavelength range. The reason for the significant difference in flux between MBs and NSs could be
because MBs (unlike NSs) are related to incoherent generation of Langmuir waves. The nature of the MB emission is similar
to the smoothly varying (background) emission of the NSs, butthe MB emission is impulsive because of the high rate of pitch-angle
diffusion. 相似文献
74.
为获取岩石在破裂过程中的动态应力场,首先进行室内物理试验获取声发射数据,在此基础上基于能量耗散原理,利用实测声发射信息建立起岩石细观损伤表征方程,并通过FLAC3D内嵌FISH语言进行二次开发,自动搜索声发射损伤影响范围内岩石单元并对其力学参数进行弱化,计算得到较为真实的岩石破裂动态应力场。结果表明,计算得到的岩石破裂应力场与实测结果有良好的对应关系,验证了岩石细观损伤表征方法的合理性。同时,获得的岩石动态破裂应力场不仅可以从岩石力学的角度解释破坏产生的原因,也对预测岩石下一步破坏具有指导意义。但这种方法仍具有一定的局限性,需要进一步的探索研究。 相似文献
75.
高压密闭消解-电感耦合等离子体光谱和质谱联合测定海洋地质样品中52种元素 总被引:4,自引:0,他引:4
An improved analytical method to determine the content of 52 major, minor and trace elements in marine geological samples, using a HF-HCl-HNO_3 acid system with a high-pressure closed digestion method(HPCD), is studied by an inductively coupled plasma optical emission spectrometry(ICP-OES) and an inductively coupled plasma mass spectrometry(ICP-MS). The operating parameters of the instruments are optimized, and the optimal analytical parameters are determined. The influences of optical spectrum and mass spectrum interferences, digestion methods and acid systems on the analytical results are investigated. The optimal spectral lines and isotopes are chosen, and internal standard element of rhodium is selected to compensate for matrix effects and analytical signals drifting. Compared with the methods of an electric heating plate digestion and a microwave digestion, a high-pressure closed digestion method is optimized with less acid, complete digestion,less damage for digestion process. The marine geological samples are dissolved completely by a HF-HCl-HNO_3 system, the relative error(RE) for the analytical results are all less than 6.0%. The method detection limits are 2–40μg/g by the ICP-OES, and 6–80 ng/g by ICP-MS. The methods are used to determine the marine sediment reference materials(GBW07309, GBW07311, GBW07313), rock reference materials(GBW07103, GBW07104,GBW07105), and cobalt-rich crust reference materials(GBW07337, GBW07338, GBW07339), the obtained analytical results are in agreement with the certified values, and both of the relative standard deviation(RSD) and the relative error(RE) are less than 6.0%. The analytical method meets the requirements for determining 52 elements contents of bulk marine geological samples. 相似文献
76.
粉尘释放是风蚀造成危害的一个重要过程。以农牧交错带沙区和非沙区农田土壤为研究对象,利用室内风洞模拟实验,实时监测了风蚀过程中释放的PM10,分析了PM10的动态变化特征,以深入认识土壤风蚀粉尘释放机理。结果表明:非沙区农田土壤风蚀强度远低于沙区农田,与风速呈指数函数关系;非沙区农田的土壤粉尘释放在不同风速下均以气流直接抬升模式为主,平均PM10通量与风速呈线性函数关系,最大PM10通量与风速呈幂函数关系;沙区农田的土壤粉尘释放在风速增大到一定程度后呈气流直接抬升和砂粒跃移冲击复合模式,最大PM10通量增加不明显,但平均PM10通量明显高于非沙区农田;对于沙区和非沙区农田而言,平均PM10通量与风蚀速率呈对数函数关系。 相似文献
77.
应用全球多部门、多区域动态可计算一般均衡(CGE)模型,采用情景分析方法,评估美国退出《巴黎协定》后,由于其碳排放路径的变化对国际气候谈判中的3个重要谈判方中国、欧盟和日本实现国家自主贡献(NDC)和2℃目标情景下碳排放空间和减排成本的影响。结果表明:在全球碳排放固定且分配方式固定的条件下,美国不同程度的退约将为自身获得较大的碳排放空间,同时挤压其他地区,包括中国、欧盟和日本实现NDC和2℃目标的碳排放空间,将推高中国、欧盟和日本实现NDC和2℃目标的碳价。2030年,2℃目标下中国碳价的升幅将达4.4~14.6美元/t,欧盟为9.7~35.4美元/t,日本为16.0~53.5美元/t。同时将增加中国、欧盟和日本等其他国家和地区的GDP损失。2030年,2℃目标下中国GDP损失的升幅将达220.0亿~711.0亿美元(相当于16.4~53.1美元/人),欧盟为93.5亿~321.4亿美元(相当于20.7~71.1美元/人),日本为41.3亿~134.5亿美元(相当于34.3~111.7美元/人)。 相似文献
78.
黄土在我国西北地区广泛分布,是当地垃圾填埋场封顶覆盖层的主要材料,该材料的气体渗透特性直接影响了覆盖层对填埋气释放的控制效果。利用渗析技术和自制的气体渗透系数测量装置,模拟和测试了干湿气象条件下覆盖黄土服役含水率变化及其对气体渗透系数的影响,并建立填埋气在垃圾体和覆盖层中的一维稳态运移模型,分析了覆盖层气体渗透系数和抽气速率对填埋气释放控制效果的影响。研究结果表明:渗析技术能有效模拟覆盖黄土服役含水率的变化,压实黄土试样的气体渗透系数介于10-17~10-12 m2量级,随服役含水率的增加而降低,且对于压实度比较高的黄土降低得更加明显;覆盖层底部的填埋气压随气体渗透系数的减小而增大,通过覆盖层下部的气体扩散层负压抽气等措施,可有效减小覆盖层底部气压和填埋气的释放量。 相似文献
79.
我国农村生活能源中SO2、 NOX及TSP的排放量估算 总被引:2,自引:0,他引:2
根据2004年我国不同省、市、自治区农村生活用能源的消耗量和不同燃料的污染物排放因子,估算了我国农村生活能源利用过程中的SO2、NOX、TSP排放量,并给出了分省区的排放清单和各省区不同燃料对三种污染物的贡献率,探讨了各地农村污染物排放量的影响因素。结果表明:全国农村生活能源所排放的SO2达530万吨,NOX 72万吨,TSP 390万吨。污染物排放以SO2和TSP为主,且各省、市、区污染物的排放量差别明显;各地不同能源类型对各污染物的贡献率差别较大,SO2主要来自燃煤,NOX主要来自秸秆和薪柴的燃烧,TSP主要来自秸秆的燃烧;农村生活能源结构影响其污染物排放。 相似文献
80.
道路交通节能减排途径与潜力分析 总被引:1,自引:1,他引:0
交通运输行业是仅次于制造业的第二大油品消耗行业,也是实现低碳生活发展路径的重点行业。基于交通运输部门碳排放量现状分析,本文提出了优先发展公共交通、鼓励发展小排量汽车、降低机动车单耗、控制排放物标准等四种挖潜减排途径,并利用排放量估算和情景分析相结合的方法,对我国道路交通减排潜力进行了预测。按照高中低度三种减排情景发展,测算出2015年及2020年减排量,为实现至2020年我国碳排放较2005年下降40%~45%的目标提供科学基础。研究认为:2010-2020年是中国交通运输行业高速发展阶段,要满足能源安全和温室气体减排要求,我国需要实施更严格的产业和环境政策,若强化低碳情景模式,则2015年、2020年的碳排减少量分别约为2183万t、7148万t,达到我国道路交通部门的最大减排潜力。 相似文献