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51.
The fractal characteristics of tidal creeks in the Gaizhou Beach are analyzed based on high-resolution images fusion of Landsat TM and ERS-2, and then the graphic models and characteristics of converse information tree of tidal creeks in the Gaizhou Beach are established. A calculation model is established based on the above results, and at the same time, quantitative calculation of the evolution characteristics and the diversity between the northern and the southern parts of the Gaizhou Beach is carried out. By the supervised classification of these images, distribution and areas of high tidal flats, middle tidal flats and low tidal flats in the Gaizhou Beach are studied quantitatively, and image charactistics of seashell habitats in the Gaizhou Beach and the correlation between mudflat distribution and seashell habitats are studied. At last, the engineering problems in the Gaizhou Beach are discussed.  相似文献   
52.
褐藻酸降解菌埃氏交替单胞菌(Alteromonas espejiana)菌株Al01,通过发酵培养制备褐藻酸酶.该酶作用的最适pH为7.0,最适温度为40℃,最适底物浓度为1%~2%;在离子浓度为0.5mmol/dm3时,Mn2+对酶促反应稍有促进作用,Ca2+、Hg2+则有明显的抑制作用.该酶用于裙带菜单细胞和原生质体解离时,以酶液组成为褐藻酸酶1%、纤维素酶1%,45×10-3的NaC1为渗透剂,酶解温度25℃,pH7.0,酶解3-4h效果最好.  相似文献   
53.
FORMATION AND EROSION PROCESSES OF THE LOESS PLATEAU   总被引:2,自引:0,他引:2  
IPROCESSANDZONINGOFLOESSACCUMULATIONLoessisatypicalkindofaeoliansediment,theprocessesofitsgeomorphicformationcanbesummarizedasfollows.l.lWell-distributedDustFalloutfromHighAltitudeThedustisdefinedasthefineparticles(<0.1mm)whichcanbeliftedandcarriedupasdustcloudsintheaiLIftheoriginallandsurfaceofaregionisanevenhighlandsurroundedbyriversandgullies,thefallingdustremainedonthesurfaceofthisevenhighland,butthedustfallingonslopesoftheriverandgullieswastransportedoutoftheregion.Onthet…  相似文献   
54.
南沙群岛遥感复合信息的珊瑚礁顶趋势面分析   总被引:1,自引:0,他引:1  
基于南沙海域区域地质构造的控制与珊瑚岛礁发育及其所表观的遥感信息特征,借助数学模型和电子计算机,以遥感复合信息所建立的趋势面分析系统,模拟了南沙珊瑚岛礁顶部地理数据的空间分布及其区域性变化趋势,从而对南沙珊瑚岛礁的空间分布特征作出科学的解释与区域比较.  相似文献   
55.
南沙珊瑚环礁的遥感复合信息熵与类型   总被引:2,自引:1,他引:1  
基于南沙群岛珊瑚环礁发育指数为多指标的观点,将测度出的多项相关因子的遥感复合信息数据,细分作N1,N2,…,N10个地理事件,进行了环礁信息熵分析。表征了烟值大小与干出环礁发育指数密切相关的因子,它们依次为礁顶面积(0.319)、渴湖面积(0.324)、环礁开放度(0.336)、走向(0.551)等。就此,对干出环礁发育指数提出一个新的表达式,用以划分南沙环礁发育的开放性类型。  相似文献   
56.
To explore the optimal land-use for soil carbon(C) sequestration in Inner Mongolian grasslands,we investigated C and nitrogen(N) storage in soil and soil fractions in 8 floristically and topographically similar sites which subjected to different land-use types(free-grazing,grazing exclusion,mowing,winter grazing,and reclamation).Compared with free-grazing grasslands,C and N storage in the 0-50 cm layer increased by 18.3%(15.5 Mg C ha-1) and 9.3%(0.8 Mg N ha-1) after 10-yr of grazing exclusion,respectively,and 21.9%(18.5 Mg C ha-1) and 11.5%(0.9 Mg N ha-1) after 30-yr grazing exclusion,respectively.Similarly,soil C and N storage increased by 15.3%(12.9 Mg C ha-1) and 10.2%(0.8 Mg N ha-1) after 10-yr mowing,respectively,and 19.2%(16.2 Mg C ha-1) and 7.1%(0.6 Mg N ha-1) after 26-yr mowing,respectively.In contrast,soil C and N storage declined by 10.6%(9.0 Mg C ha-1) and 11.4%(0.9 Mg N ha-1) after 49-yr reclamation,respectively.Moreover,increases in C and N storage mainly occurred in sand and silt fractions in the 0-10 cm soil layer with grazing exclusion and mowing.Our findings provided evidence that Inner Mongolian grasslands have the capacity to sequester C and N in soil with improved management practices,which were in the order:grazing exclusion > mowing > winter grazing > reclamation.  相似文献   
57.
Modeling of migrating grains on asteroid’s surface   总被引:1,自引:0,他引:1  
  相似文献   
58.
对泥河湾盆地郝家台、后沟、红崖和虎头梁4个地点湖相及其上覆沉积物样品进行了光释光年代学研究.由于中粒石英的单片再生剂量法所测光释光信号已经达到了饱和,故采用中粒混合矿物的红外激发后高温红外激发方法,并对其异常衰退进行校正,这种方法利用长石的释光信号,饱和剂量较高,且异常衰退较小,为测量老样品提供了可能性.根据红外激发后高温红外激发光释光测年结果,郝家台、后沟和红崖地区现存泥河湾湖相顶部沉积物年龄为360~420ka,虎头梁湖相顶层沉积物年龄为约270ka,而郝家台和后沟湖相沉积物上覆黄土-古土壤年龄分别为约130ka和180ka.这些测年结果表明在泥河湾地区湖相沉积物顶层及其上覆沉积物之间广泛存在一个沉积间断,且不同地点湖相沉积物侵蚀的程度不同.因此,推测现在泥河湾地区出露的湖相沉积物顶层并不是当时古湖泊消失时的沉积,即至少部分古湖泊沉积的顶部已被侵蚀.  相似文献   
59.
A new concept of three dimensional non-Keplerian trajectories with double angular momentum reversal is investigated with high performance solar sails. The main discussion of this paper is about such 3D solar inverse orbits with inner constraints. The problem is addressed in a time optimal control framework solved by an indirect method. Two typical solar inverse orbits have been achieved and presented in a 3D non-dimensional dynamic model in the Heliocentric Inertial Frame. Starting from the Earth orbit ecliptic plane, a sailcraft in the inverse orbit exhibits a butterfly shape trajectory. As such, the new orbits are symmetrical with respect to a plane which contains the Sun-perihelion line. The relation of the sail attitude angles between the two symmetrical parts of the orbits are used to reduce the simulation effort. The quasi-heliostationary property at its aphelia is demonstrated with variation of the orbital radius. Evolutions of the orbital velocity and optimal sail orientations are also outlined and discussed to benefit future design work. As is suited for space observation guaranteed by its butterfly shape, the inverse orbits are thoroughly studied in terms of the concerned parameters. The discussion of the parametric influence is ranked in order as perihelion distance r E , required maximum position z max, perihelion position z f and the sail lightness number β. Suitable ranges of each parameter are adopted to illustrate the orbital variation trend. Through numerical simulations the features of such inverse orbits are further emphasized to provide an initial reference for future researchers.  相似文献   
60.
In the current study, a double-averaged analytical model including the action of the perturbing body’s inclination is developed to study third-body perturbations. The disturbing function is expanded in the form of Legendre polynomials truncated up to the second-order term, and then is averaged over the periods of the spacecraft and the perturbing body. The efficiency of the double-averaged algorithm is verified with the full elliptic restricted three-body model. Comparisons with the previous study for a lunar satellite perturbed by Earth are presented to measure the effect of the perturbing body’s inclination, and illustrate that the lunar obliquity with the value 6.68 is important for the mean motion of a lunar satellite. The application to the Mars-Sun system is shown to prove the validity of the double-averaged model. It can be seen that the algorithm is effective to predict the long-term behavior of a high-altitude Martian spacecraft perturbed by Sun. The double-averaged model presented in this paper is also applicable to other celestial systems.  相似文献   
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