Simulation of streamwise vortices at the flaps of re-entry vehicles

The present study investigates separated flows in the flap region of the X-38 re-entry demonstrator with respect to the heat loads downstream reattachment induced by streamwise vortices. In a first step generic numerical flow simulations of turbulent ramp configurations with artificially induced vortex disturbances are compared with wind tunnel data of the Ludwieg tube facility in Göttingen (RWG). The results allow insight into the perturbed flow field, the associated flow topology and the influence of different flow parameters that affect the perturbations. For numerical resolution of streamwise vortices in the boundary layer of re-entry vehicles local grids are generated around the flaps of the X-38 vehicle. Extensive studies of arranging and refining the local grids demonstrate good grid convergence. For laminar cases and cases with fixed transition vortex effects on the heat transfer are observed with and without artificial vortex excitation.

Zusammenfassung

Ziel der vorgelegten Studie ist die Untersuchung abgelöster Strömungen im Klappenbereich des X-38 Wiedereintrittsdemonstrators hinsichtlich der durch Längswirbel entstehenden thermischen Belastungen stromab der Anlegelinie. Im ersten Schritt werden turbulente generische Rampenkonfiguratiorien mit künstlich induzierten Wirbelstörungen mit Windkanaldaten des Ludwierohrkanals in Göttingen (RWG) verglichen. Die Ergebnisse erlauben einen Einblick in die Störströmung, der zugehörige Strömungstopologie und der Einflüsse verschiedener Parametervariationen auf die Störströmung. Zur numerischen Auflösung der Längswirbel in der Grenzschicht von Wiedereintrittsvehikeln wurden lokale Netze um die X-38 Klappen generiert. Ausführliche numerische Studien nach Umordnung und Verfeinerung der lokalen Netze zeigen eine gute Netzkonvergenz der Ergebnisse. In laminaren Fällen und solchen mit fester Transition wurden Wirbeleinflüsse auf den Wärmestrom mit und ohne künstliche Wirbelanregung beobachtet.     

First millimetric detections of AE Aquarii

We report the first millimetric detections of the magnetic cataclysmic variable AE Aquarii, accompanied by contemporaneous microwave observations. These data show that the time-averaged spectrum is well fit by a power-law which extends to mm wavelengths. We suggest that the spectrum is consistent with that expected from a superposition of flare-like events.     

基于内容分析法的航空公司网站营销绩效评估

遵循服务导向的原则,从航空公司网站目标顾客的角度出发,针对信息服务、互动服务和电子商务服务等构建了评价指标体系;进而采用内容分析法,选择内地民航客运市场14家航空公司的简体中文网站进行了绩效评估;并采用非参数检验的手段,进行了进一步的实证研究。     

辽宁省城镇化内涵及其影响因素分析

城镇化是社会发展的必然趋势，是我国现代化建设的必由之路，但目前对城镇化内涵的还没有一个完整统一的认识。城镇化内涵应该包括经侪城镇化、产业结构城镇化、人口城镇化、空间城镇化、生活方式城镇化等。从城镇化的内涵人手，对其影响因素进行分析，旨在对辽宁城镇化的进程进行测量，以期进一步推动辽宁城镇化的进程。     

高超侧压式进气道参数分析及试验研究

分析了高超侧压式进气过第一、二溢流窗的溢流角随后掠角的变化规律，分析了溢流窗气流与主流相互作用而形成一道脱体曲面激波的原因，设计了侧压角为６°，后掠角３０°的直前缘及圆弧前缘两套高超侧压式进气道，在Ｍ５．３风洞中利用风洞壁面自然发展的附面层进行非均匀来流下进气道起动性能及总体性能试验，试验发现大量附面层吸入不仅对起动性能有重大影响，而且对总压恢复影响也极大。     

Composition of Light Solar Wind Noble Gases in the Bulk Metallic Glass flown on the Genesis Mission

We discuss data of light noble gases from the solar wind implanted into a metallic glass target flown on the Genesis mission. Helium and neon isotopic compositions of the bulk solar wind trapped in this target during 887 days of exposure to the solar wind do not deviate significantly from the values in foils of the Apollo Solar Wind Composition experiments, which have been exposed for hours to days. In general, the depth profile of the Ne isotopic composition is similar to those often found in lunar soils, and essentially very well reproduced by ion-implantation modelling, adopting the measured velocity distribution of solar particles during the Genesis exposure and assuming a uniform isotopic composition of solar wind neon. The results confirm that contributions from high-energy particles to the solar wind fluence are negligible, which is consistent with in-situ observations. This makes the enigmatic “SEP-Ne” component, apparently present in lunar grains at relatively large depth, obsolete. ²⁰Ne/ ²²Ne ratios in gas trapped very near the metallic glass surface are up to 10% higher than predicted by ion implantation simulations. We attribute this superficially trapped gas to very low-speed, current-sheet-related solar wind, which has been fractionated in the corona due to inefficient Coulomb drag.     

Doo-Sabin细分算法的实现

在细分曲面造型中，对Doo-Sabin曲面为代表的细分曲面的研究，已成为近几年来图形学领域最重要的研究课题，但已有文献在细分算法的实现方面缺乏具体操作过程，不便于工程应用。本文分析了Doo-Sabin细分算法的数据结构特点，研究了细分算法的具体实现过程，对连接规律进行了总结，实现了Doo-Sabin细分算法的二次曲面细分，为各种相关文献缺乏具体操作过程作了补充。     

浅析Ackermann函数

利用递归函数显式化的一种新方法,给出了Akermann函数显式表示法,从而确定Akermann函数算法的时间复杂度为2幂函数级.     

3He-Rich Solar Energetic Particle Events

³He-rich solar energetic particle (SEP) events show huge enrichments of ³He and association with kilovolt electrons and Type-III radio bursts. Observations from a new generation of high resolution instruments launched on the Wind, ACE, Yohkoh, SOHO, TRACE, and RHESSI spacecraft have revealed many new properties of these events: the particle energy spectra are found to be either power-law or curved in shape, with the ³He spectrum often being distinctly different from other species. Ultra-heavy nuclei up to >200 amu are found to be routinely present at average enrichments of >200 times solar-system abundances. The high ionization states previously observed near ∼1 MeV/nucleon have been found to decrease towards normal solar coronal values in these events. The source regions have been identified for many events, and are associated with X-ray jets and EUV flares that are associated with magnetic reconnection sites near active regions. This paper reviews the current experimental picture and theoretical models, with emphasis on the new insights found in the last few years.     

Imaging diagnostics of solar non-thermal particles

Non-thermal hard X-ray, gamma-ray and radio emission are the most direct signatures of the presence of energetic particles in the solar atmosphere. This paper lays emphasis on hard X-ray and radio imaging data, obtained during and outside flares, which reveal the sites where particles interact with the ambient medium. These observations, which provide more or less direct information on the topology and dynamics of the magnetic structures in which particles are accelerated and propagate, are discussed in the framework of the statistical flare scenario.