Small scale structures in the solar corona

The observational characteristics of the small scale magnetic structures are summarized. The temperature structure and temporal variability of the emission from coronal bright points, that pervade the source region of the solar wind in coronal holes and the quiet sun, and from active regions are shown to be remarkably similar. Particular emphasis is given to observations, potentially feasible with SOHO, that could resolve some of the outstanding issues regarding the role of the small scale magnetic structures in the energy balance and properties of the solar wind.     

端板法翼型实验的数据处理与洞壁干扰修正方法

 用端板法测量气动力数据时,端板附近有自由涡拖出。通过实验观察假设了端板翼型实验的涡系模型。由涡系模型可计算出机翼加端板后的有效展弦比,再按举力线理论可将实验结果转换成二维(翼型)数据;按镜象法也可作升力洞壁干扰修正。对于端板法中间剖面的测压结果亦应作二维转换和洞壁干扰修正,方法类似。经过这样的数据处理后,翼型数据准确可靠。     

连接翼布局直接力控制可能性的初步探索

对连接气动布局实现直接力控制的可能性进行了初步的探索。通过前、后机翼的长降舵面的不同偏转角组合，分别产生直接升力，侧力和阻力，提高了飞机的气动性能，并改善了控制的响应品质，给飞机提供了独立的姿态或轨迹控制的非同寻常的运动模态。增加头部鸭翼可进一步提高和改善了连接翼布局的直接升力特性。     

10°尖锥气动特性边界层转捩诱导量的测定研究

本文用风洞实验的方法在国内外首次测出了１０°尖锥气动特性的转捩诱导量，包括转捩诱导法向力及其作用点，转捩诱导俯仰力矩和尖锥压心的转捩诱导量。研究结果表明，这些转捩诱导量随Ｒｅ数的变化趋势合理，具有确定的规律性。研究认为，这些转捩诱导量产生的原因是细长锥边界层转捩的不对称性。利用这些结果，可以很好地解释边界层转捩何以对细长锥的气动静稳定性和气动稳定性产生极为显著的影响以及静、动稳定性转捩诱导量之间的相关现象。此外，这个研究结果还有助于证明边界层转捩将影响物面的压力分布。本研究是在Ｍ＝５，α＝０°的流场中完成的，实验的Ｒｅ数范围为ＲｅＬ＝２．８×１０６～１３．８×１０６。     

翼伞归航准则及测风原理探讨

翼伞作为一种新型气动力减速器日渐受到空间回收技术重视。文中给出了具有非比例自动归航控制的翼伞系统的归航准则(考虑到风的影响)以及利用GPS测量数据计算风场的公式。     

On the derivation of empirical limits on the helium abundance in coronal holes below 1.5R s

We present a simple technique describing how limits on the helium abundance, , the ratio of helium to proton number density, can be inferred from measurements of the electron density, temperature and their gradients below 1.5R _s. As an illustration, we apply this technique to emission line intensities in the extreme ultraviolet, measured in polar coronal holes. The example indicates that can be significantly large in the inner corona. This technique could be applicable to the more extensive data to be obtained from coordinated ground and space-based observations during the Ulysses south polar passage and the Spartan flight, and subsequently during the SOHO mission. Limits on the helium abundance in the solar wind can thus be derived from its source region and compared to interplanetary values.     

超音速风洞测压的系统统校

风洞实验中经常遇到利用多台仪器测量同一物理量的问题，而各子系统之间的一致性是影响测试准确度的重要因素。就子系统之间的误差对测压实验结果的影响进行了分析并介绍了统校方法。结果表明：子系统本身不确定度比较高，一般不低于０．１％，而多个子系统的分散度相对比较差。因此，利用多套子系统同时测量某一物理量时，有必要进行系统统校；经过统校并作适当处理后，系统的准确度明显提高，实验结果也更趋合理。     

超高空系缆气球的空气动力特性试验研究

介绍自然形状和流线形状两种高空系缆气球的空气动力特性。着重探讨攻角和雷诺数对升力、阻力和俯爷力矩的影响。指出：合理、良好的气动外形（具备可靠的稳定性和最小阻力），对提高抗风能力、增加留空时间都有重要意义。     

Unsteady aerodynamic modeling at high angles of attack using support vector machines

Accurate aerodynamic models are the basis of flight simulation and control law design.Mathematically modeling unsteady aerodynamics at high angles of attack bears great difficulties in model structure determination and parameter estimation due to little understanding of the flow mechanism.Support vector machines(SVMs)based on statistical learning theory provide a novel tool for nonlinear system modeling.The work presented here examines the feasibility of applying SVMs to high angle-of-attack unsteady aerodynamic modeling field.Mainly,after a review of SVMs,several issues associated with unsteady aerodynamic modeling by use of SVMs are discussed in detail,such as selection of input variables,selection of output variables and determination of SVM parameters.The least squares SVM(LS-SVM)models are set up from certain dynamic wind tunnel test data of a delta wing and an aircraft configuration,and then used to predict the aerodynamic responses in other tests.The predictions are in good agreement with the test data,which indicates the satisfying learning and generalization performance of LS-SVMs.     

UVCS/SOHO: The First Two Years

The SOHO Ultraviolet Coronagraph Spectrometer (UVCS/SOHO) has observed the extended solar corona between 1 and 10 R· for more than two years. We review spectroscopic and polarimetric measurements made in coronal holes, equatorial streamers, and coronal mass ejections, as well as selected non-solar targets. UVCS/SOHO has provided a great amount of empirical information about the physical processes that heat and accelerate the solar wind, and about detailed coronal structure and evolution. This revised version was published online in June 2006 with corrections to the Cover Date.