What type was SN 1987A?     

L. A. L. Da Silva 《Astrophysics and Space Science》1990,165(2):255-260

A comparison is made of the light and colour curves of the SN 1987A in the first 280 days with the mean properties of type II supernovae. The conclusion is that even though it has H lines, and was not a typical type II supernova, but a peculiar object from a photometric point of view. The implications for inclusion of SN 1987A in the context of the usual Minkowski-Zwicky classification are explicitly discussed.  相似文献   

Voids in the Jagiellonian Field     

T. Grabińska 《Astrophysics and Space Science》1985,115(2):369-376

This paper presents arguments relating to the phenomenon of scantily populated regions with intergalactic obscuration.  相似文献   

Notes on Hori Method for Canonical Systems     

Sandro Da Silva Fernandes 《Celestial Mechanics and Dynamical Astronomy》2003,85(1):67-78

In this paper a slightly different approach is proposed for the process of determining the functions S _m and H _m ^* of the algorithm of the canonical version of Hori method. This process will be referred to as integration theory of the mth order equation of the method. It will be shown that the ordinary differential equation with an auxiliary parameter t ^* as independent variable, introduced through Hori auxiliary system, can be replaced by a partial differential equation in the time t. In this way, the mth order equation of the algorithm assumes a form very similar to the one of other perturbation methods. In virtue of this new approach of the integration theory for Hori method, Lagrange's variational equations introduced by Sessin are revised. As an example, the Duffing equation is solved through this new approach.  相似文献   

Energy interconnection between the plasma cloud ejected from the active region and the shock wave     

I. N. Garczyńska  B. Rompolt 《Solar physics》1986,105(1):101-109

The relation between the ejected plasma cloud and the shock wave propagating ahead of it is examined for 27 pairs of such events. The flare sprays and the eruptive prominences observed in H line as well as the fast-moving sources of type-IV radio bursts have been considered as such ejected plasma clouds. Propagation of the shock wave in the solar corona has been examined from the observations of type-II radio bursts. Using the Parker model of the propagation of a shock wave, the shock wave velocity has been compared with the plasma cloud velocity. Energy interconnection between these two events has been studied. In the majority of the investigated cases there exists an energetic interconnection between the plasma cloud and the shock wave.  相似文献   

Transfer of60Co from midwater squid to sperm whales     

Takeshi Umezu  Hiroshi Ebihara  Yōko Minamisako  Hiroshi Watanabe 《Journal of Oceanography》1984,40(5):382-390

Sperm whales are notable squid-eaters. They feed mainly on medium to large-sized cephalopods at midwater levels and defecate near the surface. This suggests the existence of an upward transport of⁶⁰Co by sperm whales from the mesopelagic zone (150–1,200 m). To elucidate this squid-whale route for this artificial radionuclide,⁶⁰Co content was determined in squid and in predator whales captured by commercial whaling. In the Cephalopoda livers⁶⁰Co levels of 30–500 mBq kg^–1 wet were found and in the viscera of Odontoceti (toothed whales) 15–40 mBq kg^–1 wet. About 0.3% of⁸⁰Co ingested was estimated to be retained in a 23-year-old male sperm whale. In the livers of Bryde's whales,⁶⁰Co levels of 40–80 mBq kg^–1 wet were detected, but not in euphausiids and sardines, their possible prey. The level of Co in sperm whales was nearly the same as in Bryde's whales. Specific radioactivity⁶⁰Co/⁵⁹Co in mBq µg^–1 was several times higher in sperm whale (1.1–1.6) than in cephalopods (0.19–0.77). Eating prey with a high content of⁶⁰Co in the 1960's may have contributed to the present body burden in sperm whales with a long-life span. However, the origin of⁶⁰Co in Bryde's whales is unknown.  相似文献   

Magnetic anomalies in the canary basin and the Mesozoic evolution of the central North Atlantic     

W. R. Roest  J. J. Dañobeitia  J. Verhoef  B. J. Collette 《Marine Geophysical Researches》1992,14(1):1-24

The data from a recent magnetic compilation by Verhoefet al. (1991) off west Africa were used in combination with data in the western Atlantic to review the Mesozoic plate kinematic evolution of the central North Atlantic. The magnetic profile data were analyzed to identify the M-series sea floor spreading anomalies on the African plate. Oceanic fracture zones were identified from magnetic anomalies and seismic and gravity measurements. The identified sea floor spreading anomalies on the African plate were combined with those on the North American plate to calculate reconstruction poles for this part of the central Atlantic. The total separation poles derived in this paper describe a smooth curve, suggesting that the motion of the pole through time was continuous. Although the new sea floor spreading history differs only slightly from the one presented by Klitgord and Schouten (1986), it predicts smoother flowlines. On the other hand, the sea floor spreading history as depicted by the flowlines for the eastern central Atlantic deviates substantially from that of Sundvik and Larson (1988). A revised spreading history is also presented for the Cretaceous Magnetic Quiet Zone, where large changes in spreading direction occurred, that can not be resolved when fitting magnetic isochrons only, but which are evident from fracture zone traces and directions of sea floor spreading topography.Deceased 11 November 1991  相似文献   

水中矿物油荧光特性实验研究     

夏达英  张士魁  李宝华  王振先  孙培光  史锦珊  尚丽平 《海洋科学进展》2002,20(2):91-98

为了实现现场测量地表水中矿物油含量的全光纤荧光计的研制。采用荧光光谱测量分析方法 ,于 1 999年 1 0月— 2 0 0 0年 5月 ,采集了国内外不同的地区原油和成品油共 2 3种 ,用1 4种不同波长的激发光激励 ,进行荧光光谱特性测量实验研究。同时 ,对不同浓度的矿物油、水混合液也进行了测量实验 ,得出其最低检测浓度为 0 .0 0 5mg/L ;测量了青岛近岸海域表层受油污染海水的含油量为 0 .0 1～ 0 .2 2mg/L ;此外对水中矿物油受激荧光发射原理也作了简述。并对水中矿物油荧光光谱特性、浓度与荧光强度的关系 ,以及为研制现场测量水中矿物油浓度的全光纤荧光计的可能性作出了结论性的意见  相似文献   

影响单位进尺成本的因素及其影响规律研究   总被引：1，自引：0，他引：1  

张伟  王达 《地质科技情报》2008,27(3):93-97

介绍了一种用于分析不同因素对单位进尺成本影响的新方法--偏因素分析方法,该方法可用于在影响因素众多的情况下确定各因素对施工经济性的影响作用;同时介绍了成本影响系数这一新概念,成本影响系数表示了某一因素在一定的条件下对单位进尺成本影响程度的大小.在钻进技术经济研究中采用成本影响系数,可使对影响单位进尺成本因素的对比评价更加方便易行.以一个5 000 m取心钻进项目为例,计算了不同影响因素变化时的单位进尺成本和成本影响系数,最终根据成本影响系数绝对值的大小,对影响单位进尺成本的不同因素进行了评价.  相似文献   

Structure features of convective channels from thermal sources in Mutnovskii volcano (South Kamchatka)     

Yu. A. Manshtein  S. B. Bortnikova  A. K. Manshtein  G. M. Gavrilenko  I. V. Vernikovskaya  N. P. Sez’ko 《Doklady Earth Sciences》2008,423(2):1404-1409

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Extension of the solution of Kepler's equation to high eccentricities     

Sandro Da Silva Fernandes 《Celestial Mechanics and Dynamical Astronomy》1994,58(3):297-308

The classic Lagrange's expansion of the solutionE(e, M) of Kepler's equation in powers of eccentricity is extended to highly eccentric orbits, 0.6627 ... <e<1. The solutionE(e, M) is developed in powers of (e–e*), wheree* is a fixed value of the eccentricity. The coefficients of the expansion are given in terms of the derivatives of the Bessel functionsJ _n (ne). The expansion is convergent for values of the eccentricity such that |e–e*|<(e*), where the radius of convergence (e*) is a positive real number, which is calculated numerically.  相似文献