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721.
根据红移定义1+z=λi/λ0i,我们认为类星体红移分布ln(1+z)周期性受两个因素影响。首先,决定类星体红移的主要线(如Lα1216,CIV1549,CIII1909,MgII2798,NeV3426,OII3727,NeIII3868,Hγ4340,Hβ4861,OIII5007)固有波长可能构成0.205的周期性;另外,这些谱线的观测波长进入一定光学窗口对红移有一定限制,在一定条件下,它正好在某些红移出现峰值,并与ln(1+z)=0.205预言峰值一致。我们还在这两个基本考虑下进行模拟取样,发现有明显周期性,定量上证实了我们的基本考虑。本文是类星体红移分布的一种解释,它能说明为什么统计分布不同样品能得到不同的结论。进而,我们认为红移分布周期性不能成为内禀红移观点的观测支持。 相似文献
722.
A linear regression analysis of 28 selected tide-gauge stations of the Zhujiang Estuary shows that there has been a tendency of local sea level rise at a rate of 2.028 mm per year. The origin of the variation is significantly attributed to the local tectonic movement of discrepant fault-block. Based on this, four types of relative local sea level changes are classified. According to calculation, half of the fertile land, or 800 km2 of the delta plain will have been submerged by sea water by about 2040. This will yield a significant influence on the economic construction and human activities. 相似文献
723.
This paper presents a two-dimensional, Alfvén-wave-driven solar wind model, in which the wave energy is assumed to cascade from the low-frequency Alfvén waves to high-frequency ion cyclotron waves and to be transferred to the solar wind protons by cyclotron resonance at the Kolmogorov rate. A typical structure in the meridional plane consisting of a coronal streamer near the Sun, a fast wind in high latitudes, and a slow wind across the heliospheric current sheet, is found. The fast wind obtained in the polar region is essentially similar to that derived by previous one-dimensional flow-tube models, and its density profile in the vicinity of the Sun roughly matches relevant observations. The proton conditions at 1 AU are also consistent with observations for both the fast and slow winds. The Alfvén waves appear in the fast- and slow-wind regions simultaneously and have comparable amplitudes, which agrees with Helios observations. The acceleration and heating of the solar wind by the Alfvén waves are found to occur mainly in the near-Sun region. It is demonstrated in terms of one-dimensional calculations that the distinct properties of the fast and slow winds are mainly attributed to different geometries of the flow tubes associated with the two sorts of winds. In addition, the 2-D and 1-D simulations give essentially the same results for both the fast and the slow winds. 相似文献
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Initial results of centralized autonomous orbit determination of the new-generation BDS satellites with inter-satellite link measurements 总被引:3,自引:0,他引:3
Chengpan Tang Xiaogong Hu Shanshi Zhou Li Liu Junyang Pan Liucheng Chen Rui Guo Lingfeng Zhu Guangming Hu Xiaojie Li Feng He Zhiqiao Chang 《Journal of Geodesy》2018,92(10):1155-1169
Autonomous orbit determination is the ability of navigation satellites to estimate the orbit parameters on-board using inter-satellite link (ISL) measurements. This study mainly focuses on data processing of the ISL measurements as a new measurement type and its application on the centralized autonomous orbit determination of the new-generation Beidou navigation satellite system satellites for the first time. The ISL measurements are dual one-way measurements that follow a time division multiple access (TDMA) structure. The ranging error of the ISL measurements is less than 0.25 ns. This paper proposes a derivation approach to the satellite clock offsets and the geometric distances from TDMA dual one-way measurements without a loss of accuracy. The derived clock offsets are used for time synchronization, and the derived geometry distances are used for autonomous orbit determination. The clock offsets from the ISL measurements are consistent with the L-band two-way satellite, and time–frequency transfer clock measurements and the detrended residuals vary within 0.5 ns. The centralized autonomous orbit determination is conducted in a batch mode on a ground-capable server for the feasibility study. Constant hardware delays are present in the geometric distances and become the largest source of error in the autonomous orbit determination. Therefore, the hardware delays are estimated simultaneously with the satellite orbits. To avoid uncertainties in the constellation orientation, a ground anchor station that “observes” the satellites with on-board ISL payloads is introduced into the orbit determination. The root-mean-square values of orbit determination residuals are within 10.0 cm, and the standard deviation of the estimated ISL hardware delays is within 0.2 ns. The accuracy of the autonomous orbits is evaluated by analysis of overlap comparison and the satellite laser ranging (SLR) residuals and is compared with the accuracy of the L-band orbits. The results indicate that the radial overlap differences between the autonomous orbits are less than 15.0 cm for the inclined geosynchronous orbit (IGSO) satellites and less than 10.0 cm for the MEO satellites. The SLR residuals are approximately 15.0 cm for the IGSO satellites and approximately 10.0 cm for the MEO satellites, representing an improvement over the L-band orbits. 相似文献
728.
Acta Geotechnica - Given copper and lead mine enrichment and the high yield of North-Western China, the metallurgical industry attains prosperity. Metallurgical industrial waste which contains... 相似文献
729.
Acta Geotechnica - Interlocking refers to a kind of resistance caused by the staggered arrangement of granular materials. In geotechnical engineering, it is considered as one of the important... 相似文献
730.
采用岩石薄片鉴定、X射线衍射分析、扫描电镜以及元素地球化学等分析测试手段,对罗布泊盐湖罗北凹地杂卤石的沉积和分布特征进行了研究。结果显示,罗北凹地杂卤石主要发育于含盐系中上部,或以质地较纯的层状杂卤石岩产出,或与钙芒硝/石盐/白钠镁矾共同产出。杂卤石有交代和原生两种成因类型:前者是罗北凹地杂卤石产出的主要类型,是罗布泊硫酸盐型盐湖自身蒸发析出产物,在盐湖演化中后期交代钙芒硝或者石膏形成;后者可能为富钙卤水补给富钾镁盐湖形成。罗北凹地杂卤石的分布具有在南北方向上南厚北薄、在东西方向上中间厚两侧薄的特点,对应的KCl含量也同样具有南高北低、中间高两侧低的特点,它们的分布特征明显受控于区域构造活动,构造导致的沉降区有利于杂卤石聚集成矿。本区杂卤石矿埋藏浅、规模较大,可作为后备钾盐资源。 相似文献