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311.
312.
利用放射性示踪沙定量观测长江口北槽航道抛泥区底沙运动 总被引:3,自引:0,他引:3
1991年6月在国际原子能机构的合作下,在长江口北槽航道上抛泥区进行了一次大规模的放射性示踪沙试验。示踪核素为钪-46,总活度为17.95×10~(10)Bq(4.85Ci),示踪沙投放总量为495g。本试验目的是通过定量观测底沙运移的方向、路线、速度和输沙率,以期为北槽航道上抛泥区今后能否继续作为抛泥区使用提供直观可靠论据。本次试验观测资料表明,在北槽航道上抛泥区,在中小讯期间,无论是涨潮时投放的示踪沙还是落潮时投放的示踪沙都受落潮流控制,并向北槽航道中段输移。据测量资料分析,在上口抛泥区投放的示踪沙最终沿着110°的运动方向以758m/d的运动速度,在269~#航标附近进入挖槽,单宽输沙率为47.8m~3/md。 相似文献
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实验确定了分析白酒中含氮杂环化合物的最佳条件:含氮杂环化合物在pH1~2的条件下成盐,酒样浓缩10倍后以乙醚萃取除去中性杂质和酸性杂质,将样品pH再调至9,用乙醚萃取后KD浓缩,取样品进行气相色谱分析。以上述条件测定了茅台酒等6种名酒中的含氮化合物,发现各种酒中均有含氮杂环化合物存在,但因酒型的差别,化合物含量和组成模式相差较大。 相似文献
315.
Gas chromatographic determination of lignin in sediment 总被引:1,自引:0,他引:1
After the oxidation of river and marine sediments with CuO under alkaline conditions, the phenolic compounds in the oxidation products are determined gas chromatographically and compared to that of lignin oxidation products. The method of CuO oxidation is compared to that of nitrobenzen. The quantitative determination of produced phenolic compounds by capillary gas chromatography is examined and the blank and repetibility of the method are tested. 相似文献
316.
LP估计在星载GPS运动学定轨中的应用及精度分析 总被引:2,自引:0,他引:2
为得到高精度的星载GPS运动学定轨,必须利用观测精度高的相位观测值,但是相位观测值预处理后,仍然存在残余小周跳.在残差服从正态分布情况下LS法是最佳参数解算方法,但该方法不能解决资料的系统误差消除问题,LP估计是处理资料残差分布含有系统误差的有效方法之一.基于LS、LP方法的有效条件和GPS数据预处理的特性,将LP估计方法引入星载GPS运动学定轨数据处理中,以CHAMP卫星资料为例,研究了LP估计在星载GPS运动学定轨中的应用及其精度分析.实践表明:在处理含有残余小周跳的相位观测值时,LP估计比LS更有效,提高了星载GPS运动学定轨精度,但随着残余周跳的进一步修复,LP估计相对于LS估计的优越性越来越弱,在资料完全没有系统误差,残差服从正态分布的情况下,LP估计不能很好地体现其优越性,精度反而低于LS估计. 相似文献
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V. A. Shefer 《Astronomy Letters》2007,33(4):270-282
We suggest a new approach to solving the problem of finding the orbit of a celestial body from its three spatial position vectors and the corresponding times. It allows most of the perturbations in the motion of a celestial body to be taken into account. The approach is based on the theory of intermediate orbits that we developed previously. We construct the orbit the motion along which is a combination of two motions: the motion of a fictitious attracting center whose mass varies according to Mestschersky’s first law and the motion relative to the fictitious center. The first motion is generally parabolic, while the second motion is described by the equations of the Gylden-Mestschersky problem. The constructed orbit has such parameters that their limiting values at any reference epoch define a superosculating intermediate orbit with a fourth-order tangency. We have performed a numerical analysis to estimate the accuracy of approximating the perturbed motion of two minor planets, 145 Adeona and 4179 Toutatis, by the orbits computed using two-position procedures (the classical Gauss method and the method that we suggested previously), a three-position procedure based on the Herrick-Gibbs equation, and the new method. Comparison of the results obtained suggests that the latter method has an advantage. 相似文献
319.
The 40Ar/39Ar dating of alteration muscovite from the Peak Au mine in the Early Devonian Cobar Basin, New South Wales, has distinguished two major episodes of mineralization. Veined (Pb‐Zn‐Cu‐Au) mineralization was broadly synchronous with cleavage formation during the post‐inversion, shortening deformation of the basin sedimentary rocks, and replacive Ag‐Pb‐Zn mineralization significantly postdates the latter event. Veined base metals (Pb‐Zn‐Cu) and Au associated with silicification were coeval with three stages of cleavage formation (D1, D2 and D3) after basin inversion. The Cu‐Au phase of mineralization at the Peak Au mine which was broadly contemporaneous with the culmination of the cleavage‐forming events (D3) and with the local development of high‐strain zones occurred at 401.5 ± 1.0 Ma (40Ar/39Ar on muscovite). This date is essentially coeval with known fossil constraints on the age of basin formation, and indicates that basin inversion and deformation rapidly followed sedimentation. In contrast, replacive Ag‐Pb‐Zn mineralization occurred at 384.0 ± 1.4 Ma (40Ar/39Ar on muscovite) during an extended period of relaxation characterized by normal faulting (D4) which followed the shortening deformation. This mineralization was associated with desilicification and chlorite‐muscovite replacement assemblages which cross‐cut the cleavages, and which may have been broadly contemporaneous with the deposition of part of the Mulga Downs Group which unconformably overlies the Cobar Supergroup. Rhyolite exposed in the core of the Peak Au mine largely contains inherited zircons that range in age from ~430–1500 Ma. A few euhedral zircons have an age of ~430 Ma and this is interpreted as a maximum date for the rock. Zircons from a syn‐D3 chlorite‐muscovite replacement zone within the deposit have 206Pb/238U ages of ~410–650 Ma and are apparently inherited. 相似文献
320.
????JASON\|2????1 a?????????GPS?????????????????????в?????JASON\|2???????????λ????仯??PCV????????????????????????????????????JASON\|2??PCV?????в???????????????????PCV???JASON\|2??1 a?????????????????в????????????ζ???????JPL?????????????????????????????????????,????PCV???????JASON\|2????????????????????????????????3D RMS???2.5 cm??????RMS?1.0 cm???????? 相似文献