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1.
利用上海天文台的照相底片资料,确定了疏散星团NGC6530天区364颗恒星的自行和成员概率,并对有关自行测定的方法、结果和精度等问题作了较为详细的介绍和讨论。使用的底片历元差为87年,全部恒星自行中误差的均方根值为1.09mas/a。 相似文献
2.
Wen Shengchang 《海洋学报(英文版)》1988,7(3):325-343
The method developed by Wen et al. (1988 a) for deriving theoretical wind wave frequency spectrum in deep water is extended to the case of water of finite depth, in which a parameter η=H/d is introduced, where H and d represent the average wave height and water depth respectively. The derived spectra reduce to those in deep water when η=0. The case of η=1/2 corresponds to waves impending to break because of the effect of the bottom. Simplified forms of spectra are given. The theoretical results agree with the observed spectra well. 相似文献
3.
In contrast with the usual method to obtain the wind-wave directional spectrum by multiplying the frequency spectrum with an empirical directional function, the authors attempt to derive analytically the directional spectrum by adopting proper spectral form and using effective parameters, namely, the zero order momentm
0 of the wind-wave frequency spectrumS(), its peak frequency 0 and the so-called peakness factorP=0
S(0)/m
0, where is angular frequency. The directional spectrum is given in a form of frequency spectrum for each direction. The spectral directionality depends on, in addition to frequency, the wind-wave growth status, for the peakness factorP as introduced by the authors previously is a measure of the wave development stage. The salient features of the directional spectrum, comparison with existing formulas and the verification of the spectrum by observational data are to be given in the Part 2 of the paper.Project supported by the National Natural Science Foundation of China. 相似文献
4.
Wen Shengchang 《海洋学报(英文版)》1988,7(1):1-16
In this part ot the paper theoretical wind-wave spectra nave been derived oy (I) expressing the spectrum in series composed of exponential terms; (2) assuming that the spectrum satisfies a high order linear ordinary differential equation; (3) introducing proper parameters in the spectrum; and (4) making use of some known charateristics of wind-wave spectrum, for instance, the law governing the equilibrium range. The spectrum obtained contains the zero order moment of the spectrum m0, the peak frequency ω0 and the ratio R =ω/ω0 (ω being the mean zero-crossing frequency) as parameters. The shape of the nondimensional spectrum S(ω) = ω0S(ω)/m0(ω=ω/ω0) changes with R and theoretically reduces to a Dirac delta function δ(ω-1) when R = 1. A spectrum of simplified form is given for practical uses, in which R is replaced by a peakness factor P=S(1). 相似文献
5.
伶仃洋L_2和L_(16)孔第四纪有孔虫群与孢粉化石带特征及其地质意义 总被引:5,自引:0,他引:5
本文所依据的分析样品是取自珠江最大的一个河口湾伶仃洋中部的水下钻孔岩芯,其底部到达花岗岩基底。通过对第四纪有孔虫群与孢粉化石带特征的分析,阐明在相同的钻孔岩芯中,有孔虫分布变化所反映的古沉积环境特征与孢粉分析的古气候特征较为吻合,并与相应的沉积相对应,结合 ̄(14)C和 ̄(230)Th/ ̄(232)Th比值法测年数据,从而较好地重塑本区晚更新世中期以来的地质历史。 相似文献
6.
TOGA—COARE强化观测期间,对赤道暖池区海流作了多种方法、多层次的观测;根据美国释放的漂流浮标不同时刻位置的资料,分别对赤道及其南、北海域的表层漂流状况作了计算分析,指出:从1°N向北存在单一的北向流;从1°N~1°S这个近赤道区域内为东向流;1°N~2°S区域为过渡区,以东向流为主,个别浮标出现涡旋状运动。2°S以南为一反时针运动的大涡旋。 相似文献
7.
气候转型与早期人类迁徙 总被引:4,自引:0,他引:4
目前的旧石器考古证据表明,更新世早期可能发生了两次人类迁徙浪潮,时间分别在1.8-1.6MaBP和1.0MaBP左右,第一阶段,古人类演化为直立人并开始走出非洲、迁徙至其它中低纬度的热带-亚热带地区;第二阶段,直立人开始占据中高纬度的温带和干旱-半干旱地区。这两个阶段也是第四纪气候发生转型、环境产生重大调整的时期。二者在发生时间上的一致性揭示了它们之间的内在联系,推测气候转型时期环境转变是这两次人类迁徙浪潮的主要驱动力。 相似文献
8.
Wen Yuh Lee 《Marine environmental research》1978,1(1):5-17
Two series of experiments were carried out to assess the long-term effects of the water soluble fractions (WSF) of fuel oils on the marine isopod, Sphaeroma quadridentatum. In one experiment, juvenile isopods (one month old) were exposed to sublethal concentrations (0·1% to 15% WSF) of a fuel oil (Baytown, Exxon) at room temperatures of 24 ± 1–6°C for nine months. These isopods survived to maturity and reproduced. However, growth rate was adversely affected at concentration ≥ 3% WSF and fecundity was depressed at concentrations ≥ 1% WSF. Survival of offspring in clean seawater was dependent to a large extent on the history of the previous generation. Offspring from groups exposed to ≥ 1% WSF experienced high mortality (> 70% within five weeks) even in clean seawater. This may imply that a population of Sphaeroma exposed to WSF as low as 0·2 ppm may eventually disappear, although animals can grow to maturity and reproduce at concentrations < 3 ppm.In another experiment, adult Sphaeroma (three months old) were subjected to the WSFs of four fuel oils (Baton Rouge, Baytown, Montana and New Jersey) for one month. Fecundity was depressed at a concentration > 15% WSF, regardless of the kind of fuel oil. On the other hand, the number of young produced bythe surviving females varied with the type of fuel oil for the same level of WSF. This may be attributed to different relative amounts of toxic components present in the WSF. 相似文献
9.
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