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951.
Y.‐C. Wei C.‐M. Zhang Y.‐H. Zhao Q.‐H. Peng X.‐J. Wu J. Wang Y.‐Y. Pan H.‐X. Yin Y. Yan T.‐S. Yan H.‐J. Tian A. Esamdin A.L. Luo Y. Cai A. Taani 《Astronomische Nachrichten》2010,331(8):817-831
Under the two initial 1‐D one parameter velocity distribution forms (one is normal, the other is exponential), the z direction scale height evolution of normal neutron stars in the Galaxy is studied by numerical simulation. We do statistics for the cases at different time segments, also do statistics for the cumulative cases made of each time segment. The results show in the cumulative cases the evolution curves of the scale heights are smoother than in the each time segment, i.e., the cumulation improve the signal‐to‐noise ratio. Certainly the evolution cases are different at different Galactic disk locations, which also have very large difference from the average cases in the whole disk. In the initial stages of z evolution of normal neutron stars, after the beginning transient states, the cumulative scale heights increase linearly with time, and the cumulative scale height increasing rates have linear relationship with the initial velocity distribution parameters, which have larger fluctuation in the vicinity of the Sun than in the whole disk. We utilize the linear relationship of the cumulative scale height increasing rates vs. the initial velocity distribution parameters in the vicinity of the Sun to make comparison with the observation near the Sun. The results show if there is no magnetic decay, then the deserved initial velocity parameters are obvious lower than the present well known results from some authors; whereas if introducing magnetic decay, for the 1‐D normal case we can make consistence among concerning results using magnetic decay time values which are supported by some authors, while for the 1‐D exponential case the results show the lackness of young pulsar samples in the larger z in the vicinity of the Sun (© 2010 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim) 相似文献
952.
To investigate the dependence of the Holmberg effect of paired galaxies on three-dimensional separations, we have constructed
four subsamples characterized by three-dimensional separations s ≤ 50 kpc, 50 kpc < s ≤ 100 kpc , 100kpc < s ≤150kpc , and
150 kpc < s ≤ 200 kpc , respectively. In this study, linear correlation coefficients and surplus standard deviations of color
indices, luminosity, and size between two components of paired galaxies are calculated. It is found that there is a weak tendency
for correlation coefficients of color indices to increase with decreasing three-dimensional separations, but such a tendency
does not exist for ones of luminosity and size. We also note that there is no tendency for surplus standard deviations to
decrease with decreasing three-dimensional separations. This suggests that it is still very difficult to clearly affirm the
dependence of the Holmberg Effect of paired galaxies on three-dimensional separations. 相似文献
953.
Zn2+对日本沼虾(Macrobrachium nipponensis)的急性致毒效应 总被引:1,自引:0,他引:1
在水温(27.4±1.3)℃条件下,以体长(33.23±1.66)mm、体质量(0.7893±0.1518)g的日本沼虾为实验动物,采用静水停食法开展了Zn2+对日本沼虾的急性毒性实验,并以此为基础,测定了Zn2+不同质量浓度水平下日本沼虾的耗氧率与窒息点.结果表明:(1)Zn2+对日本沼虾的急性致死效应与其呼吸生理代谢受阻密切相关;(2) Zn2+对日本沼虾24h、48h、72h、96h的半致死质量浓度依次为1.493、0.844、0.643和0.464mg/L; (3) Zn2+对日本沼虾昼均、夜均和日均耗氧率均无显著影响的阈值为0.046mg/L,该值为Zn2+对日本沼虾急性毒性的安全质量浓度;(4) Zn2+对日本沼虾产生轻度胁迫和中度胁迫的质量浓度范围分别为0.046-0.064mg/L和0.064-0.082mg/L. 相似文献
954.
Prorocentrum donghaiense is one of the most common red tide causative dinoflagellates in the Changjiang (Yangtze) River Estuary and the adjacent area of the East China Sea. It causes large-scale blooms in late spring and early summer that lead to widespread ecologic and economic damage. A means for distinguish- ing dinoflagellate blooms from diatom (Skeletonema costatum) blooms is desired. On the basis of measure- ments of remote sensing refectance [Rrs(λ)] and inherent optical parameters, the potential of using a mul- tispectral approach is assessed for discriminating the algal blooms due to P. donghaiense from those due to S. costatum. The behavior of two reflectance ratios [R1 = Rrs(560)/Rrs(532) and Re = Rrs(708)/Rrs(665)], suggests that differentiation of P. donghaiense blooms from diatom bloom types is possible from the current band setup of ocean color sensors. It is found that there are two reflectance ratio regimes that indicate a bloom is dominated by P. donghaiense; (1) R1 〉 1.55 and R2 〈 1.0 or (2) R1 〉 1.75 and R2 ≥ 1.0. Various sensitivity analyses are conducted to investigate the effects of the variation in varying levels of chlorophyll concentration and colored dissolved organic matter (CDOM) as well as changes in the backscattering ratio (bbp/bp) on the efficacy of this muitispectral approach. Results indicate that the intensity and inherent op- tical properties of the algal species explain much of the behavior of the two ratios. Although backscattering influences the amplitude of Rrs(λ), especially in the 530 and 560 nm bands, the discrimination between P. donghaiense and diatoms is not significantly affected by the variation of bbp/bp. Since aCDOM (440) in coastal areas of the ECS is typically lower than 1.0 m-1 in most situations, the presence of CDOM does not interfere with this discrimination, even as SCDOM varies from 0.01 to 0.026 nm-1. Despite all of these effects, the dis- crimination of P. donghaiense blooms from diatom blooms based on multispectral measurements of Rrs(λ) is feasible. 相似文献
955.
956.
957.
气象卫星观测资料全球交换的基础——FM94 BUFR码原理及实现 总被引:1,自引:1,他引:0
针对风云二号(02)批应用系统项目建设中气象卫星观测资料全球交换的需求,介绍了FM94 BUFR码的压缩原理、BUFR编码软件的信息结构和软件结构,并以风云二号C星云导风产品BUFR编码为例,给出了报文段3的详细内容和段4的数据宽度。编码结果表明BUFR编码有较高的数据压缩率,非常适合数据传输。 相似文献
958.
959.
960.
古生产力是指地质历史时期生物在能量循环过程中固定能量的速率。陆相盆地古生产力的研究包括古生产力的大小及其组成研究两个方面。目前主要通过有机碳、生物硅和生物标志化合物等指标来评估陆相盆地古生产力的大小;通过生物标志化合物指标,包括正烷烃、萜类、甾类分子标志化合物等指标来研究陆相盆地古生产力的组成。陆相盆地古生产力的定量化研究比较欠缺,仅在有机碳、生物硅及生物标志化合物指标方面建立了数学模型,且多是对海相盆地古生产力指标的直接沿用;而在色素、湖相碳酸盐等具陆相特点的指标方面仅见部分定性研究。在地学应用方面,以陆相盆地古生产力研究为基础的地球生物学方法,在正演陆相烃源岩的形成过程研究中具有良好的前景。 相似文献