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91.
SARAL/AltiKa has a Dual Frequency Microwave Radiometer (DFMR), and Jason-2 has an Advanced Microwave Radiometer (AMR). Both microwave radiometer sensors include a 23.8 GHz primary water sensing channel. The measurement consistencies between DFMR and AMR are important for establishing a consistent altimetry data set between SARAL/AltiKa and Jason-2 in order to accurately assess sea level rise in a long-term time series. This study investigates the measurement consistency in the 23.8 GHz channel between DFMR and AMR at the Simultaneous Nadir Overpasses (SNO's) between the two satellites and also at coldest ocean brightness temperature locations. Preliminary results show that while both instruments show no significant trends over the one year since the launch of SARAL, a consistent relative bias of 2.88 K (DFMR higher than AMR) with a standard deviation of 0.98 K is observed. The relative bias at the lowest brightness temperature from the SNO method (-3.82 K) is consistent with that calculated from coldest ocean method (-3.74 K). The relative bias exhibits strong latitude (and scene temperature) dependency, changing from -3.82 K at high latitudes to -0.92 K near the equator. There also exists an asymmetry between the northern and southern hemisphere. The relative bias increases toward the lower end of brightness temperature. 相似文献
92.
93.
Jian Cao Zhijun Jin Wenxuan Hu Yijie Zhang Suping Yao Xulong Wang Yueqian Zhang Yong Tang 《Marine and Petroleum Geology》2010
Calcite veins and cements occur widely in Carboniferous and Permian reservoirs of the Hongche fault zone, northwestern Junggar Basin in northwest China. The calcites were investigated by fluid inclusion and trace-element analyses, providing an improved understanding of the petroleum migration history. It is indicated that the Hongche fault behaved as a migration pathway before the Early Cretaceous, allowing two oil charges to migrate into the hanging-wall, fault-core and footwall reservoirs across the fault. Since the Late Cretaceous, the Hongche fault has been sealed. As a consequence, meteoric water flowed down only into the hanging-wall and fault-core reservoirs. The meteoric-water incursion is likely an important cause for degradation of reservoir oils. In contrast, the footwall reservoirs received gas charge (the third hydrocarbon event) following the Late Cretaceous. This helps explain the distribution of petroleum across the fault. This study provides an example of how a fault may evolve as pathway and seal over time, and how reservoir diagenetic minerals can provide clues to complex petroleum migration histories. 相似文献
94.
研究了连续变量函数的全局最优化问题 ,给出了动态隧道方法。该动态隧道方法由局部搜索和动态隧道 2个阶段构成。在局部搜索阶段用了动态系统方法。对全局最优化问题的实例进行了数值实验 ,数值结果表明了该方法的稳健性和有效性。 相似文献
95.
振动性能是评估鱼雷动力系统优劣的重要指标。将鱼雷动力舱段抽象为由振源、传递路径、响应点构成的集中参数动力学模型,在频域内对动力学方程推导,得到了系统的稳态响应幅值表达式。结合电气系统的插入损失概念,提出了适用于评估鱼雷动力舱段隔振元件效果的速度插入损失指标。结合工程问题给出了算例,表明在设计初期可以清晰地规划动力舱段的隔振结构的性能参数。 相似文献
96.
本文简要介绍了云南天文台10 米口径的太阳射电望远镜天线的远程控制系统中局域网控制和通过电话线控制的实现方案 相似文献
97.
Xiao-Qing Wen Hong Wu Chen Cao Xiao-Yang Xia Department of Physics Tianjin Normal University Tianjin National Astronomical Observatories Chinese Academy of Sciences Beijing 《中国天文和天体物理学报》2007,7(2):187-198
We made model fitting to the mid-to-far infrared spectral energy distributions (SEDs) for different categories of galaxies in the main extragalactic field of the Spitzer First Look Survey with the aid of spectroscopic information from the Sloan Digital Sky Survey. We find that the mid-to-far infrared SEDs of HII galaxies, mixture type galaxies and LINERs can be well fitted by the one-parameter (α) dust model of Dale et al. plus the 13 Gyr dust-free elliptical galaxy model. The statistics of α values indicates that all these galaxies tend to be quiescent, although the HII galaxies are relatively more active than the LINERs. The mid- infrared SEDs of absorption galaxies are well fitted simply by the 13 Gyr dust-free elliptical galaxy template, and the near-to-mid infrared SEDs of QSOs can be represented by AGN NGC 5506. 相似文献
98.
在柱坐标下将黑子周围的环形区域(黑子除外)内的振荡分解为朝向黑子传播的(入射的)波和离开黑子传播的(出射的)波。对无黑子的环形区域内的振荡也进行了同样的分解。将黑子周围的入射波看成是被黑子磁流管磁化了的介质(介质内的磁场基本是水平的)中的波。而无黑子区的入射波看成是非磁化介质中的波。比较这两种波在固定波数下功率随频率的分布发现,在磁化介质中不同径向除n的声波(p模)频率系统降低,同时功率也降低,降低的功率最高达非磁化介质中波的功率的30%。而比较在固定频率下功率随波数的分布发现,磁场中f模及n=1,2,3的p模的脊向高波数方向位移,功率的降低受频率调制,即声波在某些有限的频带中被吸收。这些观测表明,在磁场中p模与磁声重力波(MAG)产生了模式混合或耦合。模式混合的存在支持了模式转换作为p模式被黑子吸收的机制的解释。此外,本文还分析了转换的MAG波进入黑子磁流管(其中的磁场基本上是垂直的)后进一步被吸收,吸收的功率最高达MAG波的20%。在磁流管内没有进一步观测到模式的转换 相似文献
99.
本文用1970-1995年的冕洞资料,分析了冕洞的分布规律,磁场极性的演化特征和冕洞的地磁效应,以及它们与太阳黑子周期的演化关系,得到了一些有意义的结论。特别指出赤道冕洞和极区冕洞具有相反的演化规律和不同的特征。 相似文献
100.
We explore the hard X-ray source distributions of an C1.1 flare occurred on 14 December 2007. Both Hinode/EIS and RHESSI observations are used. One of EIS rasters perfectly covers the double hard X-ray footpoints, where the EUV
emission appears strong from the cool line of He ii (log T=4.7) to the hot line of Fe xvi (log T=6.4). We analyze RHESSI X-ray images at different energies and different times before the hard X-ray maximum. The results
show a similar topology for the time-dependent source distribution (i.e. at 14:14:35 UT) as that for energy-dependent source distribution (i.e. at a given energy band of 6 – 9 keV) overlapped on EUV bright kernels, which seems to be consistent with the evaporation
model. 相似文献