Residual noise covariance for Planck low-resolution data analysis

Aims: Develop and validate tools to estimate residual noise covariance in Planck frequency maps. Quantify signal error effects and compare different techniques to produce low-resolution maps. Methods: We derive analytical estimates of covariance of the residual noise contained in low-resolution maps produced using a number of map-making approaches. We test these analytical predictions using Monte Carlo simulations and their impact on angular power spectrum estimation. We use simulations to quantify the level of signal errors incurred in different resolution downgrading schemes considered in this work. Results: We find an excellent agreement between the optimal residual noise covariance matrices and Monte Carlo noise maps. For destriping map-makers, the extent of agreement is dictated by the knee frequency of the correlated noise component and the chosen baseline offset length. The significance of signal striping is shown to be insignificant when properly dealt with. In map resolution downgrading, we find that a carefully selected window function is required to reduce aliasing to the sub-percent level at multipoles, ell > 2Nside, where Nside is the HEALPix resolution parameter. We show that sufficient characterization of the residual noise is unavoidable if one is to draw reliable contraints on large scale anisotropy. Conclusions: We have described how to compute the low-resolution maps, with a controlled sky signal level, and a reliable estimate of covariance of the residual noise. We have also presented a method to smooth the residual noise covariance matrices to describe the noise correlations in smoothed, bandwidth limited maps.

Simulation of precipitation reactions in reverse micelles

Precipitation involving mixing of two sets of reverse micellar solutions-containing a reactant and precipitant respectively-has been analyzed. Particle formation in such systems has been simulated by a Monte Carlo (MC) scheme (Li, Y.; Park, C. W. Langmuir 1999, 15, 952), which however is very restrictive in its approach. We have simulated particle formation by developing a general Monte Carlo scheme, using the interval of quiescence technique (IQ). It uses Poisson distribution with realistic, low micellar occupancies of reactants, Brownian collision of micelles with coalescence efficiency, fission of dimers with binomial redispersion of solutes, finite nucleation rate of particles with critical number of molecules, and instantaneous particle growth. With the incorporation of these features, the previous work becomes a special case of our simulation. The present scheme was then used to predict experimental data on two systems. The first is the experimental results of Lianos and Thomas (Chem. Phys. Lett. 1986, 125, 299, J. Colloid Interface Sci. 1987, 117, 505) on formation of CdS nanoparticles. They reported the number of molecules in a particle as a function of micellar size and reactant concentrations, which have been predicted very well. The second is on the formation of Fe(OH)(3) nanoparticles, reported by Li and Park. Our simulation in this case provides a better prediction of the experimental particle size range than the prediction of the authors. The present simulation scheme is general and can be applied to explain nanoparticle formation in other systems.

NMR study of ammonium halides under high pressure

Wide-line c.w. proton resonance investigations have been carried out on the ammonium halides, namely, ammonium chloride, ammonium bromide and ammonium iodide in the temperature range between 77 and 300 K and in the pressure range between 1 bar and 14 kbar. It has been found that the narrow iodide spectrum at 77 K broadens under the application of hydrostatic pressure. The barrier height for the ammonium ion motion in ammonium iodide under pressure has been estimated by carrying out a temperature variation study. The rotational potential for the motion of ammonium ion in ammonium iodide at 1 bar and 14 kbar has been calculated using earlier theoretical models and compared with values calculated for ammonium chloride and bromide. The barrier height in the case of ammonium iodide under pressure is found to be of the same order of magnitude as the value obtained in the case of ammonium bromide at atmospheric pressure indicating that the high pressure phase of ammonium iodide is likely to have the same structure as the low temperature ordered CsCl phase found in the case of the chloride and the bromide. The increase in the potential barrier height in the case of ammonium iodide under pressure indicates that the reorientational motion executed by the ammonium ions is inhibited by the application of pressure. This is also confirmed by the broadening of the spectral line at 77 K under the application of pressure.

Your water resources

(26 page document)

A short survey of the environment at the dumping site for Santa Cruz Harbor dredging and A study of seaward dipping internal structures in marine ripple marks at Whaler's Cove, California. Annual report, Part 4, August 1972

(PDF contains 76 pages)

Final report on an inventory of flowing artesian wells in Florida: leading to the enforcement of sections 373.021 - 373.061 Florida Statutes 1957

This report published as Information Circular No. 21, together with the interim report published in 1957 as Information Circular No. 10, Florida Geological Survey, illustrates as completely as possible the situation that now exists among the freely flowing wells of the State. (PDF contains 40 pages.)

Grazing by manatees excludes both new and established wild celery transplants: Implications for restoration in Kings Bay, FL, USA

We conducted a field experiment between August 2001 and February 2002 in Kings Bay, FL, USA, designed to determine whether the amount of time allowed for wild celery (Vallisneria americana Michx) transplants to establish altered the effect of herbivorous manatees (Trichechus manatus L.)on their survival.

航天器编队飞行的动力学解析分析与阵形设计研究

随着微电子、微机械技术的进步，现代航天器逐渐向体积小、重量轻的趋势发展。结构的轻型化和小型化使得微小航天器在制造和发射上的成本大大降低，同时也使得微小航天器难以独立携带复杂的载O如何开发和利用多颗微小航天器的集群功能来完成复杂的航天任务已日趋成为各航天机构的研究热点，航天器编队飞行即是在这种背景下应运而生的。所谓航天器编队飞行，是指若干颗航天器在整个任务期间都按一定的几何形状排列和飞行，以实现资源共享、信息共享，共同完成某一特定功能。研究表明，航天器编队飞行可用于实现多种功能，如绕飞监视、天基合成孔径雷达、天基干涉仪、电子侦察及卫星导航等。诚然，若人为地施加燃料控制，航天器群可以实现所有的几何构型，然而付出的代价是巨大的。本文立足于最大限度地利用航天器的自然轨道特征，而非通过不断消耗燃料的方法实现航天器群的编队飞行。航天器编队飞行实质上对于航天器群的相对运动提出了一定的约束条件，因此充分地研究两航天器之间的相对运动是进行航天器编队设计的理论基础。然而，这一理论基础与航天器编队飞行所需结论之间仍存在很远的距离。本文在航天器相对运动的理论基础上，通过解析分析的方法研究了航天器编队飞行所需解决的一系列问题，例如：如何选择可行的编队阵形，如何在满足编队飞行约束条件下，进行航天器群的轨道设计。首先，本文在不考虑摄动力情况下，建立了两个航天器相对运动的微分方程，并得到了描述两航天器相对运动的解析解；其次，针对目前文献广泛应用的C-w���程及其解进行了理论分析，指出C-W���程解应用于编队飞行设计的局限性，即只能适用于近圆轨道近距离航天器的编队飞行设计；针对实际航天应用中常遇到的椭圆轨道航天器编队及远距离航天器编队，本文从相对运动解析解出发，经过一系列的数学推导与分析，导出了相应的编队设计公式；然后，本文考虑了环境摄动力如地球非球形摄动力、大气阻力、太阳光压力、第三引力体引力对于编队阵形的影响，以及摄动力情况下编队阵形的保持问题；最后，以卫星导航应用为例，利用本文导出的远距离编队公式设计了我国领土范围内的区域连续导航卫星系统，通过与目前的北斗卫星导航系统相比较，充分展示了航天器编队飞行的特点与应用优势。本文的创新之处体现在如下几方面：1、从理论上分析了目前广泛应用于编队飞行研究的C-W���程及其解的适用范围和局限性。2、将航天器编队飞行设计从近距离拓展至远距离，并针对名义航天器运行于圆轨道的情况，导出了名义航天器飞行方向远距离编队设计公式和大偏心率大相对倾角远距离编队设计公式。3、针对名义航天器运行于任意偏心率椭圆轨道，推导出近距离编队设计公式，并提出了5种新型编队阵形。4、首次在频域范围内研究航天器相对运动规律，突破了一般轨道参数法将航天器相对运动轨迹在近圆轨道近距离范围内进行泰勒展开的传统思路。

铁基激光熔覆合金设计及微观组织与性能研究

本文设计并制备了具有优良的强韧性能和高温性能的激光熔覆涂层。利用 SEM、TEMEY X－射线衍射仪等研究了涂层的化学成分、宏微观结构及其转变机制，同时研究了涂层强韧性及耐高温磨损性能及其影响机制。对激光溶覆涂层进行了合金化、微观组织、强韧化机制、加工工艺性能设计。合金系为 Fe-Cr-C-W-Ni，成分配比（质量分数），Fe:52-60%, Cr:24-30%, C:5-6%, W:4.5-7.5%, Ni:5-6%。强化机制为两相强化、亚结构强化及固溶强化，其中强化相为合金碳化物，基体相为合金元素过饱和度极高的韧性奥氏体。亚共晶及过共晶组织的领先凝固相分别为奥氏体及 M_7C_3 合金碳化物，两相共晶组织均为韧性相奥氏体和强化相 M_7C_3 合金碳化物。加工工艺控制领先凝固相的结构、组织演化及力学性能。熔覆组织在高温时效过程中形成大量新的碳化物。在过饱和奥氏体内部，可弥散析出细小的 Mc���M_2C 及 M_(23)C_6碳化物；在奥氏体与 M_7C_3 相界面，亚稳相M_7C_3发生原位转变，形成 M_(23)C_6 及 M_6C���化物。激光熔覆合金具有较高的综合力学性能，熔覆涂层有高的显微硬度、优良的抗回火稳定性、显著的二次硬化特征、优异的抗磨粒磨损和冲击磨损性能。Fe-Cr-C-W-Ni 激光熔覆合金具有较低的裂纹形成倾向和良好的表面成形性能，这与奥氏体较高的高温韧塑性及合金的低熔点共晶特征密切相关；实验及理论分析表明，通过调整合金成分、激光工艺参数和后续热处理工艺，可获得具有不同强韧性能的熔覆涂层。

Magnetospheric access of solar particles and the configuration of the distant geomagnetic field

The access of 1.2-40 MeV protons and 0.4-1.0 MeV electrons from interplanetary space to the polar cap regions has been investigated with an experiment on board a low altitude, polar orbiting satellite (OG0-4).

A total of 333 quiet time observations of the electron polar cap boundary give a mapping of the boundary between open and closed geomagnetic field lines which is an order of magnitude more comprehensive than previously available.

Persistent features (north/south asymmetries) in the polar cap proton flux, which are established as normal during solar proton events, are shown to be associated with different flux levels on open geomagnetic field lines than on closed field lines. The pole in which these persistent features are observed is strongly correlated to the sector structure of the interplanetary magnetic field and uncorrelated to the north/south component of this field. The features were observed in the north (south) pole during a negative (positive) sector 91% of the time, while the solar field had a southward component only 54% of the time. In addition, changes in the north/south component have no observable effect on the persistent features.

Observations of events associated with co-rotating regions of enhanced proton flux in interplanetary space are used to establish the characteristics of the 1.2 - 40 MeV proton access windows: the access window for low polar latitudes is near the earth, that for one high polar latitude region is ~250 R_⊕ behind the earth, while that for the other high polar latitude region is ~1750 R_⊕ behind the earth. All of the access windows are of approximately the same extent (~120 R_⊕). The following phenomena contribute to persistent polar cap features: limited interplanetary regions of enhanced flux propagating past the earth, radial gradients in the interplanetary flux, and anisotropies in the interplanetary flux.

These results are compared to the particle access predictions of the distant geomagnetic tail configurations proposed by Michel and Dessler, Dungey, and Frank. The data are consistent with neither the model of Michel and Dessler nor that of Dungey. The model of Frank can yield a consistent access window configuration provided the following constraints are satisfied: the merging rate for open field lines at one polar neutral point must be ~5 times that at the other polar neutral point, related to the solar magnetic field configuration in a consistent fashion, the migration time for open field lines to move across the polar cap region must be the same in both poles, and the open field line merging rate at one of the polar neutral points must be at least as large as that required for almost all the open field lines to have merged in 0 (one hour). The possibility of satisfying these constraints is investigated in some detail.

The role played by interplanetary anisotropies in the observation of persistent polar cap features is discussed. Special emphasis is given to the problem of non-adiabatic particle entry through regions where the magnetic field is changing direction. The degree to which such particle entry can be assumed to be nearly adiabatic is related to the particle rigidity, the angle through which the field turns, and the rate at which the field changes direction; this relationship is established for the case of polar cap observations.

Condições de saúde bucal em atletas dos XV Jogos Pan-Americanos e III Jogos Parapan-Americanos, Rio de Janeiro, Brasil, 2007

O estudo epidemiológico transversal randomizado objetivou avaliar condições de saúde bucal nos competidores dos XV Jogos Pan-Americanos (JPA) e III Jogos Parapan-Americanos (JPPA), 2007. Foram enviados convites para 5.662 atletas (JPA) e 1.300 (JPPA). Radiografias panorâmicas digitais (RPD) foram utilizadas para o exame de triagem nos 2 eventos, e nos JPPA, os atletas também foram submetidos à avaliação do sangramento gengival interdental (SI) através de uma versão modificada do Índice de Sangramento Interdental de Eastman (EIBI). Foram obtidas RPDs de 410 atletas dos JPA, média de idade 24,38 (dp5,35), 55% homens; e de 118 dos atletas dos JPPA, média de idade de 32,3 (dp9,53), 77,97% homens. 121 competidores (JPPA) foram avaliados para SI: 78,51% homens, média de idade 32,6(dp9,6), e foram separados em grupos (G), conforme sua deficiência física: GI c/ deficiência visual (DV), com 2 subgrupos: GI-a: DV tardia e GI-c-: DV congênita/precoce; GII- deficiência de membro superior; com 1 subgrupo: GII-t: deficiência/ausência bilateral; GIII- deficiência de membro inferior (grupo controle). As RPDs foram examinadas por 1 examinador com o Kodak Dental Imaging(v6.7). A frequência e a distribuição do SI foram calculadas, e os grupos foram comparados. Resultados da triagem com RPDs, representados por número de observações(média por atleta) JPA//número de observações(média por atleta JPPA: Dentes erupcionados/ hígidos: 9097(22,19)//2451(20,77); Ausentes: 803(1,96 //405(3,43); Não erupcionados ou impactados: 330(0,80)//52(0,44); Parcialmente erupcionados e/ou hígidos: 109(0,27)//20(0,17); C��rie extensa: 261(0,64)//62(0,53); C��rie extensa e lesão periapical: 96(0,23)//50(0,42); Tratamento endodôntico e lesão periapical: 24(0,06)//13(0,11); Restaurados: 2298(5,60)//670(5,68); Imagens radiolúcidas patológicas circunscritas: 23(0,06)//0; Raízes-residuais: 27(0,07)//22(0,19); Implantes:6(0,01)//5(0,04); Dentes anteriores fraturados: 13 (0,03)//3(0,03); Molares bandados: 26(0,06)//11(0,09); Dentes anômalos: 7(0,02)//12(0,10). Resultados para SI: G-I>G-III (p=0.0002);GI-c>GI-a (p=0,042). Homens exibiram > freqüência de SI (3,6%+1,7) que mulheres (0,8%+0,5), p<0,01. Conclusões: Os dados das 2 populações de atletas mostraram que há uma grande variação na saúde bucal entre os indivíduos avaliados. Diversas condições com potencial de influenciar o desempenho esportivo dos atletas foram detectadas através de radiografias panorâmicas digitais, sugerindo que um programa de saúde bucal deve ser incluído como parte da preparação destes indivíduos.A avaliação da frequência e distribuição de sangramento gengival interdental em uma população de atletas que competiu nos III Jogos Parapan-Americanos, revelou que o tipo de deficiência ou limitação física dos competidores é um fator que influencia na saúde gengival desses indivíduos. O planejamento de um programa de saúde bucal para esta população deve ser adaptado às diferentes limitações de cada atleta.

Adaptive response of Peruvian Hake to overfishing

Compensatory mechanisms of the Peruvian hake population (Merluccius gayi peruanus) in response to heavy exploitation and changes in species interaction are discussed. Changes in the rate of cannibalism, diet composition, maximization of fecundity and behavioral adaptation are noted.

Length-weight relationships of bivalves from coastal waters of Korea

Parameters a and b of the length (L)-weight (W) relationship W = a · Lb are presented for 17 commercial bivalve species collected from the southwest coastal waters of Korea. Estimates of b varied between 2.44 (Atrina pinnata japonica) and 3.31 (Scaphara broughtonii) with a mean of 2.891 (± 0.212). A total of 2 107 specimens were analyzed for this study. The length-weight relationship was isometric in most of the species.