虾塘充气增氧精养高产试验

虾塘鼓风机充气增氧精养高产试验,目前在我国很少见到报道。 鉴于当今养虾业日趋严重的虾病危害,又缺乏经济、有效的防治办法,在对虾养殖活动中实行精养高产,面临重重困难。为另辟蹊径,以求既能防止病害,又能达到高产高效的     

逆方法最优解确定九州近海流速、流量

日本以南海域的调查研究,过去已有不少报道[1~3].众所周知,东海黑潮、西太平洋水和九州沿岸水在九州附近海域交汇,近年来,这里一直是中日黑潮合作调查研究[4]的重点海区之一这些工作显示,日本以南海域的基本特征表现为黑潮路径的大弯曲及其伴生的大冷水团和黑潮两侧中尸度涡的消长过程等等,同时表明确定该海区的流速、流量是探讨以上特征的主要内容之一以往多数作者是采用动力计算方法来确定黑潮相对流速、流量.大家知道,动力计算在不同的参考零面下所得的结果是不同的,这在黑潮强流区表现得尤为明显[5].     

Radiometry of near-earth asteroids

We report 10 micrometers infrared photometry for 22 Aten, Apollo, and Amor asteroids. Thermal models are used to derive the corresponding radiometric albedos and diameters. Several of these asteroids appear to have surfaces of relatively high thermal inertia due to the exposure of bare rock or a coarse regolith. The Apollo asteroid 3103, 1982 BB, is recognized as class E. The Jupiter-crossing Amor asteroid 3552, 1983 SA, is confirmed as class D, but low albedos remain rare for near-Earth asteroids.     

FPAR的Monte Carlo模拟研究

FPAR (fraction of photosynthetically active radiation absorbed by the canopy)是植被冠层阻截太阳光合有效辐射的比例,是遥感估算陆地生态系统植被净第一性生产力(NPP)的重要参数.利用Monte Carlo方法模拟光子在植被冠层中的辐射传输过程,以植被冠层二向反射分布函数的模拟来验证模拟的正确性;在此基础上对400-700nm光合作用波段范围内的植被叶片吸收光子辐射比例的FPAR进行模拟.FPAR的Monte Carlo模拟结果,揭示了FPAR与太阳天顶角及植被冠层参数之间的关系.     

苗儿山矿田花岗岩型高品位铀矿成矿环境及控制条件

(1)透镜状菱形断块及其对花岗岩型高品位铀矿床的控制 走滑叠接带所形成的透镜状菱形断块是花岗岩型高品位铀矿床最普遍、最重要的成矿构造场地.矿床定位于菱形断块内,如苗儿山矿田由新宁一资源断裂的次一级控制断裂双瓜断裂、天金断裂、香草坪断裂、茶狮断裂、孟沙断裂呈向北撒开,由南收敛的走滑带状叠接,形成东西高角度对倾、具地堑式正断层组合的菱形断块,控制了沙子江、双滑江及孟公界等高品位铀矿床分布(图1).     

Plasma processing of interstellar PAHs into solar system kerogen

Processes resulting in the formation of hydrocarbons of carbonaceous chondrites and the identity of the interstellar molecular precursors involved are an objective of investigations into the origin of the solar system and perhaps even life on earth. We have combined the resources and experience of an astronomer and physicists doing laboratory simulations with those of a chemical expert in the analysis of meteoritic hydrocarbons, in a project that investigated the conversion of polycyclic aromatic hydrocarbons (PAHs) formed in stellar atmospheres into alkanes found in meteorites. Plasma hydrogenation has been found in the University of Alabama at Birmingham Astrophysics Laboratory to produce from the precursor PAH naphthalene, a new material having an IR absorption spectrum (Lee, W. and Wdowiak, T.J., Astrophys. J. 417, L49-L51, 1993) remarkably similar to that obtained at Arizona State University of the benzene-methanol extract of the Murchison meteorite (Cronin, J.R. and Pizzarello, S., Geochim. Cosmochim. Acta 54, 2859-2868, 1990). There are astrophysical and meteoritic arguments for PAH species from extra-solar sources being incorporated into the solar nebula, where plasma hydrogenation is highly plausible. Conversion of PAHs into alkanes could also have occurred in the interstellar medium. The synthesis of laboratory analogs of meteoritic hydrocarbons through plasma hydrogenation of PAH species is underway, as is chemical analysis of those analogs. The objective is to clarify this heretofore uninvestigated process and to understand its role during the origin of the solar system as a mechanism of production of hydrocarbon species now found in meteorites. Results have been obtained in the form of time-of-flight spectroscopy and chemical analysis of the lab analog prepared from naphthalene.     

地理研究性学习的选题策略

研究性学习是我国基础教育课程改革的一个亮点,而好的选题是研究性学习成功的一半.要迈好地理研究性学习这一步,必须熟悉地理研究性学习的选题策略--遵循科学选题的原则,学会科学选题的基本途径,关注生活中的地理知识.     

湖南及邻区地壳旋转的可能成因、对大地构造演化的影响及其与大规模成矿作用关系初探

在湖南及邻区,无论从地表的地质构造还是地球物理场上,都表现出明显的环状分布特征。这种特征可能是地壳的旋转运动所造成,它对湖南及邻区大地构造的演化、大规模成矿作用等具有重大的影响。本文对这种旋转运动的可能成因,以及所伴随的一系列地质作用、与大规模成矿作用的关系等进行了初步探讨。