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151.
It is commonly believed that comets are made of primordial material. As a consequence, they can reveal more information about
the origin of our solar system. To interpret the coma composition measurements of comet Churyumov–Gerasimenko that will be
collected by the Rosetta mission, models of the coma chemistry have to be constructed. However, programming the chemistry
of a cometary coma is extremely complex due to the large number of species and reactions involved. Moreover, such a program
needs to be very flexible as one may want to extend, change, or update the set of species, reactions, and reaction rates.
Therefore, we developed software to manage a database of species and reactions and to generate code automatically to compute
source/loss balances. This database includes the data from the UMIST database and the ion–molecule reactions collected by
V.G. Anicich. To use all these databases together, a lot of practical problems need to be solved, but the result is an enormous
source of information about chemical reactions that can be used in chemical models, not only for comets but also for other
applications. 相似文献
152.
电力负荷管理与控制系统 总被引:1,自引:0,他引:1
在电力负荷管理系统硬件的设计与实现中,着重介绍系统的两个关键部件、并路器和多路转换器,对系统数据采集编程,除介绍编程方法,利用的资源等外,还提出了远程数据采集处理后和计算机局域网联接的方法,简易可靠的镜象拷贝方法,以及提高软件运行可靠性的措施等。所研究的系统已交付抚顺电业局使用,实际运行表明,性能稳定,工作可靠,达到了预期的指标要求。 相似文献
153.
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. 相似文献154.
M. Abada-Simon A. Lecacheux T. S. Bastian J. A. Bookbinder G. A. Dulk 《Space Science Reviews》1994,68(1-4):291-292
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. 相似文献
155.
156.
157.
A. Grimberg D. S. Burnett P. Bochsler H. Baur R. Wieler 《Space Science Reviews》2007,130(1-4):293-300
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. 相似文献
158.
杨俊清 《西安航空技术高等专科学校学报》2006,24(1):29-31
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。 相似文献
159.
黄杰 《中国民航学院学报》1996,(6):65-67
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. 相似文献
160.
G. M. Mason 《Space Science Reviews》2007,130(1-4):231-242
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. 相似文献