黄金的成色

黄金的成色并不是一成不变的，它成色的高低是与成矿温度、成矿阶段、深度、时代、变质程度、水溶液及风化作用等有一定关系，我们从这些关系中可以寻找到我们找矿的捷径和依据。     

Evidence for interacting loop process in a phase of the May 16, 1981 flare

The behaviour of the flare in the period of enhancement and maximum of hard X-ray, microwave and decimetric type IV continuum is analysed. The elongation of the H ribbons and microwave source disclose that the energy release site was shifting through a system of loops with a velocity less than 200 km s^-1, and that the energy was carried down the field lines with a velocity of about 1000 km s^-1, implying the thermal conduction front mechanism of energy transport. Several processes of energy release are considered and it is concluded that an explanation in terms of succeeding interactions of neighbouring loops, involving fast reconnection of their poloidal components is in best agreement with the observations.Proceedings of the Second CESRA Workshop on Particle Acceleration and Trapping in Solar Flares, held at Aubigny-sur-Nère (France), 23–26 June, 1986.     

Emission features in the solar corona after the perihelion passage of Comet 1979 XI

On the coronograph spectrophotographic records taken on 31.372 UT, August 1979, some faint emission features were found which can be ascribed to Siii and Niii. These emissions were obviously a transient phenomena which were detected only 10 hr after the supposed fall of Comet 1979 XI in the Sun's photosphere. It cannot be excluded that the appearance of Si and Ni lines was triggered by the evaporation of dust particles with a high abundance of heavier elements in the solar corona. This assumption is also supported by intensity distribution of the Fex coronal line around the Sun's limb. The maximum coincide with the position angle of the projected path of the comet.     

中国近海海水中几种微量金属离子的分布研究

中国近海海水中的锌等微量元素，尚未进行过较为广泛而可靠的分布研究。极为零星的资料，还是近几年来在沿岸进行污染调查时，用陈旧的方法测定的。 世界海洋海水中微量元素的含量，不同文献报道的数据，常有一定的差别。这是自然变化，抑方法误差(包括所测形态)，是值得研究的。 本文采用单池示差反向极谱法，比较广泛而可靠地研究了中国近海海水中,锌等微量，元素的离子(和不稳定络合物)的地球化学分布。测定锌、铅、铜、镉时，样品不加任何试剂，因而避免了元素存在形态的转移及被测离子的带入或损失。     

东海海域海水中颗粒氨基酸(PAA)的组成与含量的分布调查研究

海水中的有机物的含量微少，约为0.5~2.0 C mg/L，但其种类复杂。其中以溶解有机物(DOM)为主，而颗粒有机物(POM)所占比例则更少。大洋海水中的POM主要来源于浮游生物等的死骸及其分解碎屑；另外还有海水中受风浪影响所进行的DOM-POM的动力平衡产物。近岸海水还受河流和大气带入的陆源尘影响。POM主要由颗粒氨基酸(PAA)组成。即由Asp、Glu、Thr、Ser、Ala、Gly、Leu、Ile、Val、Met、Cys、Tyr、Lys、His、Arg、Phe、Pro等17种氨基酸组成。它们是食碎动物的主要食物，构成海洋食物链的一环，与该水域生产力有直接联系。纪明侯等(1992)于1983年和1984年首次对青岛胶州湾海水中的颗粒氨基酸的组成和含量的变化及其季节变化进行了调查研究。并且在1982年和1984年前后对渤海湾、黄河口和长江口附近水域同样调查研究了表层海水中PAA的组成与含量分布。他们还于1981年7、8月和1982年7、8月乘“科学一号”考察船进一步研究了长江口外东中国海，包括福建省外海、济州岛附近海域和黑潮流域26°00′-33°00′N、123°00′-129°00′E范围内海域的20余个站位的表层海水和部分站位上不同水深中的PAA的组成和含量。兹将调查研究结果报道如下。     

Underwater Acoustic Image Transmission System Based on DSP

The underwater acoustic image transmission system based on the high-speed DSP device TMS320C549 has been studied.We use Goertzel algorithm for source decoding and MFSK for modulation.Turbo code is used for channel coding and decoding.The purpose is to implement underwater video image data transmission.     

渤海湾、黄河口和长江口海域海水中颗粒氨基酸含量的分布

海水中除含有大量无机物质外，还含有种类繁多，但含量很低的有机物质，其含量约为C 0.5-2.0mg/L。海水有机物质可分为溶解有机物质(DOM)和颗粒有机物质(POM)。前者为主要组分，后者所含比例很小。在大洋中POM的主要来源有:①浮游生物，尤其是浮游植物活体、死骸及其分解碎屑;②海水中进行的DOM-POM的动力平衡产物。近岸海水还受河流流入的陆地POM和大气带入的陆源尘埃的影响。POM主要由蛋白质、碳水化合物、脂类等组成。POM是食碎屑动物的良好食物，它构成海洋食物链的一环，与水域生物生产力有直接的联系。POM中蛋白质含量以颗粒氨基酸(PAA)表示。Daumas(1976)曾报道过沿岸海水中PAA含量的季节变异，纪明侯等(1992年)于1980-1981年首次对青岛胶州湾内PAA含量在不同站位和不同季节中的变化特征进行调査研究。作者等继而于1982年7月、1983年10月和1984年5、7、8月乘“金星二号”考察船前后首次研究了渤海湾、黄河口和长江口附近水域中颗粒氨基酸的组成与含量在不同站位中的分布。所得结果如下。     

海洋藻类--对付全球变暖的武器?

最近,由欧盟(则资助的研究项目(Parforce)研究人员发现了海洋藻类与气候变化之间的联系。项目研究人员发现,从海洋藻类及浮游生物释放的碘蒸汽,在海面上浓缩,形成对抗地球变暖的悬浮微粒。此悬浮微粒对地球气候变化及降     

A comparison of Hα and soft X-ray characteristics of spotless and spot group flares

A comparative analysis of spotless and spot group flares recorded at Hvar and Kanzelhöhe Observatories during the 21st cycle of solar activity is presented. The rate of occurrence of two-ribbon flares was found to be significantly higher for the spotless flares. In comparison with spot group flares of corresponding H importance, the soft X-ray peak values have been systematically lower for the spotless flares. The highest peak values and the energy released in soft X-rays was found for flares with a H ribbon protruding over a major spot umbra. It was found that the effective plasma temperatures in spotless flares have been considerably lower than the temperatures in spot group flares.