Earthquake, strong tide and global low temperature

＂La Madre＂ is a kind of upper atmospheric air current, and occurs as ＂warm phase＂ and ＂cold phase＂ in the sky of Pacific Ocean alternately. There exists this phenomenon, called ＂Oscillation Decade in the Pacific＂ （ODP）, for 20 - 30 years. It is concerned with 60 year cycle of the tides. Lunar oscillations explain an intriguing 60-year cycle in the world＇s temperature. Strong tides increase the vertical mixing of water in the oceans, drawing cold ocean water from the depths to surface, where it cools the atmosphere above. The first strong seismic episode in China was from 1897 to 1912; the second to the fifth was the in 1920-1937, 1946-1957, 1966-1980, 1991-2002, tsrectruely. The alternative boundaries of＂La Madre＂ warm phase and cold phase were in 1890, 1924, 1946 and 2000, which were near the boundaries of four strong earthquakes. It indicated the strong earthquakes closedly related with the substances＇ motion of atmosphere, hydrosphere and lithosphere, the change of gravity potential, and the exchange of angular momentum. The strong earthquakes in the ocean bottom can bring the cool waters at the deep ocean up to the ocean surface and make the global climate cold. the earthquake, strong tide and global low temperature are close inrelntion for each othen.     

制冷控制系统研制与探析

根据实际应用研制制冷控制系统,该系统采用温度测量、PID控制及PWM脉宽调制等技术实现了对目标对象的制冷处理,具有一定的应用价值。     

热带风暴之高度与风暴眼目

昔人常以热带风暴为甚浅之“骚动(Disturbance.)”。Hann气象学大全(第四版六百二十面)中尝谓热带风暴者,大气最下层之现象也,其涡旋(Vortex)所及之高度殊甚有限。E.V.Newnham夫人亦尝以热带风暴平浅为言。然究其所据,盖以热带风暴一经登陆,强度剧减,尤以过山为甚。John Eliot曾谓1876年十月之Backergunge风暴,即於孟加拉东部与阿萨密南部为高约3,000—6,000吋之邱陵所毁灭。此外Newnham夫人亦学数例,以为其说之论证。然Backergunge风暴过山立即消灭一事,固不足以例一切之台     

热带浮游植物将被迫“搬家”去极地?

浮游植物指悬浮于水中的微小藻类植物,是浮游生物中的自养生物部分。浮游植物广泛存在于河流、湖泊和海洋中,多分布于水域的上层,个体极小,需要用显微镜才能观察到,繁殖极快。在淡水中主要是蓝藻、绿藻、硅藻等,在海水中主要是硅藻、甲藻。     

矿物热电系数及其在地质找矿中的应用

作者的研究表明,在非本征激发区,矿物热电系数随着活化温度的增高而增大;在本征激发区,随活化温度的增高而减小。矿物晶体中所含杂质的种类和含量多少决定矿物的导电类型。矿物热电系数可广泛应用于地质找矿和矿床评价中,以黄铁矿为例,在同一水平面上的含金矿脉,矿脉中黄铁矿热电系数正值高时,其矿石含金量也高。应用黄铁矿热电系数的正高值、混合型和负值可确定矿体和矿体的剥蚀深度。     

大西洋中部地壳失踪英欲破解地表“伤口”之谜

英国卡地夫大学的科学家即将于3月5日起航，调查大西洋深处地壳失踪之谜。 通常情况下，地幔由数千米厚的地壳所覆盖，但科学家发现，在大西洋中部约有数千平方千米范围内的地壳似乎大面积失踪，地幔直接暴露在水下3000米左右的海底。卡地夫大学地球、海洋与行星科学学院的海洋地质学家克里斯认为，这有如发现了地球表面的“伤口”。他表示，该处虽不是地壳失踪的唯一之处，但可能是最为有意义的一处。一般来说，当板块撕裂后，地幔将涌出，形成岩浆。而这种通常的情况没有发生，说明一定存在某种原因。科学家希望通过调查确认该处的地壳是否从来就不存在；还是因为发生大规模地层断裂所致。如果事实果真如此，科学家希望搞清楚，这种现象是怎么形成的以及为什么会形成。[第一段]     

SOHM型氢钟在国家授时中心的运行情况分析

上海天文台研制的型号为SOHM-3和SOHM-4的3台氢原子钟在中国科学院国家授时中心(NTSC)已经运行了一年多时间。收集了每个氢原子钟与NTSC主钟的时间比对数据。数据的分析结果给出了这几台氢钟在不同采样间隔上的频率稳定度,也显示出1台氢钟明显的相位跳变,讨论了这种相位跳变的原因。比较了这3台氢钟和从美国进口的Symmetricom公司制造的氢钟的频率稳定度的温度变化效应,指出了上海天文台研究制的氢钟存在的主要问题。     

Screening and molecular classification of low-temperature protease from Antarctic microorganism and its characterization

107 strains producing protease were screened from 260 strains of Antarctic psychrophilic bacteria, among which proteolytic activity of five strains was more than 45 U ml^-1. The 16S rRNA gcne sequences homology and phylogcnetic analysis of five Antarctic psychrophillc bacteria showed that NJ276, NJS-9, NJ16-70,NJ345 belonged tO the described genus Pseudoalteromonas and NJ341 belonged to the genus Colwellia. The growth and the protease characteristic of four Antarctic psychrophilic bacteria had been studied, and the result showed that the 6ptimal temperature for growth and protease-produeing of four strains was about 10℃. Their growth and protease-produeing were still high during incubatlng 2-5 days. The maximum proteolytic activity occurred at pH 9 for four Antarctic psychrophilic bacteria. The optimal temperature of protease action of both strains NJ276 and NJ5-9 was about 50℃, however, the optimal temperature of protease aetlon of both strains NJ341 and NJ345 was about 40 ℃, and their proteolytic activity under 0℃ exhibited nearly 30% of the maximum activity, but their thermal stabilities were weaker. These results indicated that proteases from NJ341 and NJ345 were low-temperature proteases.     

大质量年轻星体新的C18O(1-0)发射

利用紫金山天文台青海观测站13.7米的毫米波望远镜对74个大质量年轻星体或候选进行了C^18O(1-0)的谱线观测。在63个源中观测到了C^18O(1-0)发射，其中57个天体第一次探测到C^18O(1-0)谱线发射。根据谱线辐射温度（TR^*)和半宽（△V），利用LTE方法计算了每个测量源的C^18O(1-0)发射的光学厚度和C^18O(1-0)分子的柱密度。讨论了^13CO(1-0)和C^18O(1-0)的谱线强度比和积分强度比。