氨氮胁迫对中华绒螯蟹(Eriocheir sinensis) 免疫功能的影响   总被引：9，自引：0，他引：9  

黄鹤忠  李义  宋学宏  王永玲  杨彩根 《海洋与湖沼》2006,37(3):198-205

在实验室条件下构建不同氨氮浓度环境和养殖时间的组间差异,研究氨氮胁迫对中华绒螯蟹免疫功能的影响。结果表明,中华绒螯蟹在NH 4-N3.0mg/L10天或1.0mg/L20天时,其血淋巴血细胞密度极显著地低于对照组(P<0.01)。NH4 -N2.0mg/L和3.0mg/L无论10天或20天,血细胞吞噬百分率均分别为显著(P<0.05)和极显著(P<0.01)地低于对照组。NH4 -N3.0mg/L10天或2.0mg/L20天,血细胞吞噬指数显著低于对照组(P<0.05)。NH4 -N1.0mg/L和2.0mg/L分别20天时,血清溶菌酶(LSZ)活力分别为显著(P<0.05)和极显著(P<0.01)地低于对照组。NH4 -N1.0—5.0mg/L10天时,血清酚氧化酶(PO)活力均极显著(P<0.01)下降;但NH4 -N1.0—4.0mg/L20天时,血清PO活力水平均比10天时有所上升。NH4 -N3.0—4.0mg/L10天或1.0—2.0mg/L20天,以及5.0mg/L10天或3.0—5.0mg/L20天时,超氧化物歧化酶(SOD)活力分别为显著(P<0.05)和极显著(P<0.01)地低于对照组。上述结果表明,随着氨氮胁迫浓度的增加和胁迫时间的延长,会引起中华绒螯蟹血细胞数量、血细胞吞噬能力、溶菌酶活力、酚氧化酶活力和超氧化物歧化酶活力等的逐渐下降,使机体非特异性免疫防御系统遭到损伤,同时机体清除自由基的能力下降,机体细胞和组织受到伤害甚至出现死亡。  相似文献   

确定任意磁性体磁化方向的样条函数法     

姜效典 《中国海洋大学学报(自然科学版)》1992,(2)

由磁异常Z_α和重力异常g,利用样条函数的微、积分性质,从泊松方程出发,直接解得磁性体的磁化方向。该方法适用于任意形状磁性体的磁异常。  相似文献   

2-D delineation of individual citrus trees from UAV-based dense photogrammetric surface models   总被引：1，自引：0，他引：1  

Ali Ozgun Ok  Asli Ozdarici-Ok 《International Journal of Digital Earth》2018,11(6):583-608

One of the challenges of remote sensing and computer vision lies in the three-dimensional (3-D) reconstruction of individual trees by using automated methods through very high-resolution (VHR) data sets. However, a successful and complete 3-D reconstruction relies on precise delineation of the trees in two dimensions. In this paper, we present an original approach to detect and delineate citrus trees using unmanned aerial vehicles based on photogrammetric digital surface models (DSMs). The symmetry of the citrus trees in a DSM is handled by an orientation-based radial symmetry transform which is computed in a unique way. Next, we propose an efficient strategy to accurately build influence regions of each tree, and then we delineate individual citrus trees through active contours by taking into account the influence region of each canopy. We also present two efficient strategies to filter out erroneously detected canopy regions without having any height thresholds. Experiments are carried out on eight test DSMs composed of different types of citrus orchards with varying densities and canopy sizes. Extensive comparisons to the state-of-the-art approaches reveal that our proposed approach provides superior detection and delineation performances through supporting a nice balance between precision and recall measures.  相似文献   

煤矿井下定向钻孔中电阻率探测技术与应用     

李博凡  刘磊  范涛  蒋齐平  王杰 《煤田地质与勘探》2022,50(1):52-58

受高瓦斯/承压奥灰水威胁的工作面开采前,一般采取定向钻进技术在工作面底板开展压裂或注浆工程保障开采安全。利用底板定向钻孔开展孔中探测工作,可更加精细揭露工作面内隐伏构造,还可实现“一孔多用”。为解决定向钻孔内的探测问题,提出一种在水平定向钻孔中进行直流电阻率法探查的方法。定向钻孔施工完毕后,退出定向钻孔施工的通缆钻杆,送入内平钻杆,将孔中高密度电缆通过钻杆尾端特制水便送入钻孔,使孔中电缆平铺于钻孔中,在定向钻孔水平段,进行孔内直流电阻率法径向探测。在理论上通过数值模拟研究层状介质下单孔测量工作模式的接收信号衰减规律、视电阻率曲线变化特征、顶底板岩性对测量结果的影响等,并采用单孔测量数据对孔旁异常范围进行反演定位。数值模拟研究表明,孔中电阻率探测方法对隐伏的异常体有良好的探测效果。通过在陕西韩城某矿井下实际煤层底板探测试验,对研究区2个定向抽采钻孔孔中探测数据进行处理,反演结果异常区与工作面内隐伏小断层位置吻合,验证了定向钻孔中电缆布置的可行性和定向钻孔内通过孔内径向和孔间透视探测隐伏构造的可靠性。   相似文献   

土壤饱和导水率空间预测的不确定性分析   总被引：3，自引：0，他引：3       下载免费PDF全文

廖凯华  徐绍辉  吴吉春  施小清 《水科学进展》2012,23(2):200-205

当土壤转换函数应用于土壤水力性质估计时,对于预测值的不确定性往往容易被忽视。为了有针对性地提出减少这种不确定性的方法和措施,提高土壤转换函数的实际应用能力,以两种现有的土壤转换函数(Vereecken和HYPRES模型)为例,将其应用于山东省平度市土壤饱和导水率的空间预测,并利用拉丁超立方抽样(LHS)方法对预测结果的不确定性进行了分析。结果表明,饱和导水率空间预测的不确定性主要来源于土壤基本性质的空间插值误差和土壤转换函数自身的预测误差。当Vereecken模型应用于饱和导水率空间预测时,预测结果的不确定性主要由土壤基本性质空间插值误差所决定,土壤转换函数预测误差的影响较小,而HYPRES模型则是受二者的双重影响。  相似文献   

小波变换压制噪声在单道地震资料处理中的应用          下载免费PDF全文

林兆彬  胡毅  郑江龙  蔺爱军 《应用海洋学学报》2018,37(1):113-119

海洋区域地质调查中,单道地震勘探以其高分辨率、方便快捷等优点成为揭示浅地层地质构造的重要手段之一.结合前人研究成果并出于保护信号的完整性,对低频部分的噪声采用带通滤波进行滤除,而对高频信号中的随机噪声采用小波阈值去噪方法进行压制处理.在小波阈值去噪过程中,通过比较选用最佳小波基函数sym5对地震剖面进行三层小波分解.结果表明:两种阈值去噪方法在带通滤波的基础上进一步提升了剖面的质量,使得反射层面变得连续可追踪.软阈值去噪滤掉了剖面上的较多信息,去噪效果较为彻底,硬阈值去噪则保留了较多的细节信息.  相似文献   

同伦函数与填充函数相结合的非线性最小二乘平差模型     

游为  范东明  傅淑娟 《武汉大学学报(信息科学版)》2010,(2)

提出了同伦函数与填充函数相结合进行非线性最小二乘平差的方法。先采用同伦函数求解非线性恰定方程组,得到一个局部最优解,然后以该局部最优解为基础构造填充函数,通过对填充函数求解,得到比当前局部最优解更小的局部极小点,再以该局部极小点为基础重新构造同伦函数和填充函数进行求解,通过有限步的循环迭代,最终找到非线性最小二乘平差的全局最优解。实例验证,该方法能有效地寻找出非线性最小二乘平差的全局最优解。  相似文献   

Nonlinear transfer function modelling of beach morphology at Duck,North Carolina     

Y. Gunawardena  S. Ilic  H. Pinkerton  R. Romanowicz 《Coastal Engineering》2009

This paper presents a simple nonlinear data-based modelling approach for predicting the beach profile volume at Duck, North Carolina, USA. The state-dependent parameter form of the general transfer function (SDP TF) model is used to describe nonlinearity influencing these morphological data in two case examples. Case 1 investigates the nonlinearity associated with the dependency of wave forcing on the preceding beach volume. Case 2 investigates the ability to model the variables within the well-known diffusion equation for beach volume using this data-based approach. The results of this study show that the SDP TF approach can be used successfully to develop statistically robust models for describing nonlinearity in beach morphological systems. Furthermore, these models are shown to predict the beach volumes over both short (1 month ahead) and long (2 years ahead) time periods, and thus show great potential for practical applications in coastal zone management and engineering.  相似文献   

A Bayesian periodogram finds evidence for three planets in HD 11964     

P. C. Gregory † 《Monthly notices of the Royal Astronomical Society》2007,381(4):1607-1616

A Bayesian multiplanet Kepler periodogram has been developed for the analysis of precision radial velocity data. The periodogram employs a parallel tempering Markov chain Monte Carlo algorithm. The HD 11964 data have been re-analysed using 1, 2, 3 and 4 planet models. Assuming that all the models are equally probable a priori, the three planet model is found to be ≥600 times more probable than the next most probable model which is a two planet model. The most probable model exhibits three periods of  38.02^+0.06_−0.05, 360⁺⁴₋₄ and 1924⁺⁴⁴₋₄₃ d  , and eccentricities of  0.22^+0.11_−0.22, 0.63^+0.34_−0.17 and 0.05^+0.03_−0.05  , respectively. Assuming the three signals (each one consistent with a Keplerian orbit) are caused by planets, the corresponding limits on planetary mass ( M sin  i ) and semimajor axis are     respectively. The small difference (1.3σ) between the 360-d period and one year suggests that it might be worth investigating the barycentric correction for the HD 11964 data.  相似文献   

WASP-1b and WASP-2b: two new transiting exoplanets detected with SuperWASP and SOPHIE   总被引：1，自引：0，他引：1  

A. Collier Cameron  F. Bouchy  G. Hébrard  P. Maxted  D. Pollacco  F. Pont  I. Skillen  B. Smalley  R. A. Street  R. G. West  D. M. Wilson  S. Aigrain  D. J. Christian  W. I. Clarkson  B. Enoch  A. Evans  A. Fitzsimmons  M. Fleenor  M. Gillon  C. A. Haswell  L. Hebb  C. Hellier  S. T. Hodgkin  K. Horne  J. Irwin  S. R. Kane  F. P. Keenan  B. Loeillet  T. A. Lister  M. Mayor  C. Moutou  A. J. Norton  J. Osborne  N. Parley  D. Queloz  R. Ryans  A. H. M. J. Triaud  S. Udry  P. J. Wheatley 《Monthly notices of the Royal Astronomical Society》2007,375(3):951-957

We have detected low-amplitude radial-velocity variations in two stars, USNO-B1.0 1219–0005465 (GSC  02265–00107 = WASP–1  ) and USNO-B1.0 0964–0543604 (GSC  00522–01199 = WASP–2  ). Both stars were identified as being likely host stars of transiting exoplanets in the 2004 SuperWASP wide-field transit survey. Using the newly commissioned radial-velocity spectrograph SOPHIE at the Observatoire de Haute-Provence, we found that both objects exhibit reflex orbital radial-velocity variations with amplitudes characteristic of planetary-mass companions and in-phase with the photometric orbits. Line-bisector studies rule out faint blended binaries as the cause of either the radial-velocity variations or the transits. We perform preliminary spectral analyses of the host stars, which together with their radial-velocity variations and fits to the transit light curves yield estimates of the planetary masses and radii. WASP-1b and WASP-2b have orbital periods of 2.52 and 2.15 d, respectively. Given mass estimates for their F7V and K1V primaries, we derive planet masses 0.80–0.98 and 0.81–0.95 times that of Jupiter, respectively. WASP-1b appears to have an inflated radius of at least 1.33 R _Jup, whereas WASP-2b has a radius in the range 0.65–1.26 R _Jup.  相似文献