Big Bang Nucleosynthesis and the Density of Baryons in the Universe

Now that extragalactic deuterium observations are being made, Big Bang Nucleosynthesis (BBN) is on the verge of undergoing a transformation. Previously, the emphasis was on demonstrating the concordance of the Big Bang Nucleosynthesis model with the abundances of the light isotopes extrapolated back to their primordial values using stellar and Galactic evolution theories. Once the primordial deuterium abundance is converged upon, the nature of the field will shift to using the much more precise primordial D/H to constrain the more flexible stellar and Galactic evolution models (although the question of potential systematic error in 4He abundance determinations remains open). The remarkable success of the theory to date in establishing the concordance has led to the very robust conclusion of BBN regarding the baryon density. The BBN constraints on the cosmological baryon density are reviewed and demonstrate that the bulk of the baryons are dark and also that the bulk of the matter in the universe is non-baryonic. Comparison of baryonic density arguments from Lyman- clouds, x-ray gas in clusters, and the microwave anisotropy are made and shown to be consistent with the BBN value.     

Early nucleosynthesis: The present situation

The most recent developments in the very light element abundance observations, especially the determination of a high (D/H) ratio 3 10^–4 on a remote QSO line of sight, are analyzed and some of the consequences on the Big Bang nucleosynthesis (BBN) models, on the predicted baryonic density and on the galactic evolution schemes are reviewed. Should this (D/H) determination be confirmed by further observations, the simplest standard BBN model would be the most successful in these abundance predictions: the baryon density should be close to the luminous mass density ^B (5–8)10^–3 if H=100 km s^–1 Mpc^–1; the challenge is now to devise galactic evolution models able to account for a large D destruction and avoiding to overproduce³He and metals.     

航路爬升性能计算

本文以 B737—300为例介绍了根据飞机及发动机的极曲线、最大爬升推力和燃油流量等原始数据及给定的爬升规律(如表速250KT/280KT/M0.74)计算在标准大气和非标准大气中航路爬升性能的方法及程序,计算结果与该机型使用手册中给出的 ISA—10,ISA,…,ISA 20的爬升数值表非常吻合。本文所述的方法及程序是通用的,对大爬升角的情况亦适用。     

Solar Models with Non-Standard Chemical Composition

The OPAL monochromatic opacity tables are used to evaluate the impact of a non-standard chemical composition on solar models. A calibrated solar model with consistent diffusion including the effect of radiative forces and ionization on drift velocities is presented. It is shown that surface abundances are predicted to change slightly more than in traditional solar models where these refinements are not included. All elements included in the model settle at similar rates which is reflected in the relative variation in surface abundances ranging from 7.5% for calcium to 8.8% for argon. The structural difference between the consistent model and the traditional model is small, with a maximum effect of 0.3% for the isothermal sound speed at the base of the convection zone. The settling of CNO is only marginally affected. Opacity profiles have also been calculated with varying abundances for volatile elements, for which the abundances are poorly known, and other selected elements. It is shown that if one allows a 10% variation of these elements individually one can expect a peak Rosseland mean opacity variation of 3% for oxygen, a little less 2% for Si and Ne, and around 1% for Mg and S in the radiative zone. Other light metals and volatile elements have no significant impact on the opacity. This revised version was published online in June 2006 with corrections to the Cover Date.     

Observations of Metals in the Intra-Cluster Medium

Because of their deep gravitational potential wells, clusters of galaxies retain all the metals produced by the stellar populations of the member galaxies. Most of these metals reside in the hot plasma which dominates the baryon content of clusters. This makes them excellent laboratories for the study of the nucleosynthesis and chemical enrichment history of the Universe. Here we review the history, current possibilities and limitations of the abundance studies, and the present observational status of X-ray measurements of the chemical composition of the intra-cluster medium. We summarise the latest progress in using the abundance patterns in clusters to put constraints on theoretical models of supernovae and we show how cluster abundances provide new insights into the star-formation history of the Universe.     

基于动态集成算法的航空发动机气路参数预测

针对单一学习机对航空发动机气路参数预测困难的问题,提出了基于动态加权核密度估计（DWKDE)组合方法的集成预测算法,该组合方法选择测试样本的近邻样本,通过评估学习机在近邻样本的局部性能动态确定各学习机的权值,并基于该权值利用加权核密度估计实现数据序列的集成预测。该组合方法不易受离群值和样本不对称分布的影响,将该组合方法用于AdaBoost.RT和AdaBoost.R2算法,获得了改进后的集成学习算法。实验证明:相比于神经网络和原始集成学习算法,改进后的集成学习算法较好地提高了航空发动机气路参数序列的预测精度,方均根误差（RMSE)指标至少可降低27%。      

Solar neutrinos: Theory versus observation

The current state of the solar neutrino problem is described. The predictions of solar models (standard and nonstandard) are reviewed. The neutrino absorption cross sections for all detectors of current interest are reviewed with special emphasis on the uncertainties that exist in the calculations for each target. A long-term program for neutrino spectroscopy of the solar interior is outlined. It is shown, in addition, that stellar collapses can be detected within the galaxy by the proposed solar neutrino detectors.     

不同电离层模型对北斗共视的精度影响分析

GNSS共视时间传递已成为远程高精度时间同步的主要技术手段之一,我国自主研制的北斗导航系统已经服务于亚太地区,基于北斗共视进行高精度时间传递已成为我国时频领域的研究热点。为了提高导航系统定位精度,需降低或消除导航定位过程中的各类误差,其中电离层为影响北斗共视的主要误差。研究了常用的几种电离层修正算法,利用2014年7月份的观测数据分析不同电离层模型对北斗共视钟差的精度影响,给出了残差标准差和稳定度值。分析结果表明:经各种电离层修正后,钟差精度都有所提高,其中双频电离层修正最优,比VTEC格网模型和Klobuchar模型分别提高22%和30%。对于不同星座,GEO卫星计算的钟差修正后精度明显优于MEO、IGSO卫星。     

一种高光谱图像的双压缩感知模型

高光谱图像因其海量数据性,给存储、传输及后续分析处理带来了挑战。压缩感知理论提供了一种全新的信号采集框架。针对高光谱数据的三维特性,提出一种双压缩感知的采样与重构模型。该模型在采样阶段兼顾高光谱数据的空间和谱间稀疏特性,构造了能同时实现空间和谱间压缩采样的感知矩阵;重构阶段不同于传统的压缩感知重构方法直接重构高光谱数据,而是将高光谱数据分离成端元和丰度分别进行重构,然后利用重构的端元和丰度信息合成高光谱数据。实验结果表明,所提双压缩感知在低采样率下重构精度较三维压缩采样提高了10 dB以上,更为显著的是运算速度提升了3个数量级,同时该方法还便于获得端元和丰度信息。     

复合材料帽形加筋结构稳定性研究

建立了复合材料帽形加筋结构的参数化有限元模型,给出了两种进行层板结合处的模拟计算方法,通过计算得到了模型的屈曲载荷并总结了加筋结构几何参数对结构稳定性的影响,给出了模型的收敛性分析,对比了模型网格密度对于计算结果的影响,找到最佳的网格密度,提高了模型计算的效率和准确性,为实际的结构设计提供了重要参考,为结构分析提供了依据。     

Video watermarking synchronization based on profile statistics

A novel temporal synchronization method for video watermarking by matching the profile statistics. The profile statistics, represented by the characteristic parameters such as position mean and variance in the x-and y-directions, of a frame in a video sequence can easily be calculated and sent as side information to the receiver. At the receiving end, temporal attacks such as transposition, dropping, and insertion can be detected by comparing side information and characteristic parameters calculated from the received video. The simulation results show that the proposed method can successfully re-synchronize the attacked video back to the original format with accuracy from 72.41% to 98.15% for various video sequences based on single frame matching. After the voting process, the GOP detection accuracy can be improved to the range of from 96.30% to 100%.     

计及高次谐波影响的高密度永磁同步电机铁耗计算

在经典Bertotti三项式常系数铁耗计算模型的基础上,基于谐波分析原理,引入涡流损耗、磁滞损耗和附加损耗补偿系数,提出了一种计及高次谐波影响的高密度永磁同步电机(PMSM)铁耗计算模型。该模型中的补偿系数均随磁密幅值、频率和畸变率变化,能较好地反映基波及谐波磁场对铁耗的影响。为了验证该模型的有效性及准确性,以48槽/8极内转子和36槽/48极外转子两台PMSM为研究对象,将模型的计算值、有限元仿真结果和试验数据进行对比分析。结果表明,铁耗计算模型有较高的精度,特别适用于磁密幅值与频率变化范围大的场合。     

辐射温度计标定误差分析

本文通过理论分析和实验,建立了标准辐射温度计和被检辐射温度计因工作波长不同而产生的标定误差公式,通过几种典型黑体空腹温度分布的测量及有效发射率的计算,讨论了分别以标准辐射温度计和接触温度计校准被检辐射温度计时误差及其走向。     

Cosmic-ray Composition as Observed by Ulysses

The cosmic ray isotopic composition measurements from the High Energy Telescope (HET) on the Ulysses spacecraft are reviewed. The source isotopic composition of key elements is found to be surprisingly like the Solar system abundances with the notable exception of ²²Ne. The average density of interstellar material cosmic rays traverse is found to be 0.25 atom cm^–3, corresponding to a confinement time of 20 Myr. Vanadium isotopic abundances are shown to be consistent with weak cosmic-ray reacceleration. The implications of these measurements are discussed.     

机载燃油密度传感器高低温静态试验技术

为了验证航空机载燃油密度传感器在高温燃油和低温燃油中的燃油密度测量精度,运用阿基米德原理对高低温静态验证试验技术进行了研究。设计和提出了一种新的高精度航空机载燃油密度传感器高低温静态试验装置和方法。研究结果表明：试验装置密度测量系统的测量最大误差为-0.077%,符合试验装置测量精度为受试品测量精度4倍及以上的规定（受试品测量精度为0.4%）。结果通过了C919总体设计单位和美国Parker公司的评审,能可靠地验证航空机载燃油密度传感器在高温燃油和低温燃油中的燃油密度测量精度,为航空机载燃油密度传感器工程应用和装机试飞提供了试验数据支撑。     

Extragalactic Abundances of Hydrogen,Deuterium and Helium New Steps,Missteps and Next Steps

Estimates of the deuterium abundance in quasar absorbers are reviewed, including a brief account of incorrect claims published by the author and a brief review of the problem of hydrogen contamination. It is concluded that the primordial abundance may be universal with a value (D/H)P 10-4, within about a factor of two, corresponding to _Bh _0.7 ² 0.0fs2 or 10 2.7 in the Standard Big Bang. This agrees with current limits on primordial helium, YP 0.243, which are shown to be surprisingly insensitive to models of stellar enrichment. It also agrees with a tabulated sum of the total density of baryons in observed components. Much lower primordial deuterium ( 2 × 10^-5) is also possible but disagrees with currently estimated helium abundances; the larger baryon density in this case fits better with current models of the Lyman- forest but requires the bulk of the baryons to be in some currently uncounted form.     

The Solar Chemical Composition

We present our current knowledge of the solar chemical composition based on the recent significant downward revision of the solar photospheric abundances of the most abundant metals. These new solar abundances result from the use of a 3D hydrodynamic model of the solar atmosphere instead of the classical 1D hydrostatic models, accounting for departures from LTE, and improved atomic and molecular data. With these abundances, the new solar metallicity, Z, decreases to Z=0.012, almost a factor of two lower than earlier widely used values. We compare our values with data from other sources and analyse a number of impacts of these new photospheric abundances. While resolving a number of longstanding problems, the new 3D-based solar photospheric composition also poses serious challenges for the standard solar model as judged by helioseismology.     

A New Algorithm for Computing Inertial Altitude and Vertical Velocity

Inertial navigators determine inertial altitude and vertical velocity by a closed feedback loop in which the vertical accelerometer output is mixed with a pressure altitude reference. Pressure altitude is determined as a function of presure based on the standard atmosphere models. Since the atmosphere is almost always nonstandard, large inertial altitude and vertical velocity errors may result. A unique algorithm has been devised to compute a dynamically corrected altitude reference by numerically integrating the physical relation for a column of air as a function of pressure, gravity, and absolute temperature. The new algorithm has been flight tested and has been shown to yield accurate results.     

确定时间序列均值和方差函数的移动多点平均方法

为了提高有限样本或小样本情况下时间序列均值和方差函数的确定精度,以保证时序建模、分析和预测精度,提出一种确定序列趋势项的移动多点平均方法.该方法能够得到时间序列均值中非周期部分,结合样本周期图法得到的周期项,可综合得到其均值函数,并可进一步得到时序的标准差函数.Monte Carlo模拟对比结果表明:该方法不仅能够保证时间序列段内分析精度,而且能够有效提高时间序列的预报精度.