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1.
H. Thiemann R. W. Schunk 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1992,12(12):143-146
Heavy emission caused by impacting plasma ions results in a fast discharging effect of the initially large surface potentials on the dielectric solar cells. This eventually counteracts the energization process of the plasma ions to the cover glasses and leaves no significant electric fields. Thus, with an existing thermal plasma, electrons are again able to reach dielectric surfaces. Strong localized electric fields of the order of several 10 kV/cm form near the interconnector-cover glass interface. 相似文献
2.
T. J. Ponman A. M. Read 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1993,13(12):361-364
Using data from the Wide Field Camera EUV all-sky survey, we have established upper limits to the EUV flux from a sample of 30 bright, nearby, non-active spiral galaxies. These galaxies were chosen to be those most likely to be detected in the EUV on the basis of (i) low interstellar absorption within our own galaxy, (ii) brightness in other wavebands, (iii) high star formation activity, and (iv) proximity. The derived EUV upper limits are restrictive, and establish for the first time that the EUV flux escaping from galaxies does not constitute a major component of their bolometric luminosity, and in particular that it cannot be the sink for the energy injected into the interstellar medium by supernova explosions, as had been suggested following the failure to detect this power in the X-ray band. 相似文献
3.
本文介绍了动态畸变测量系统及其数据处理方法.进一步提高采样频率后可将该系统用于飞机和发动机的研究中. 相似文献
4.
一种地磁匹配制导适配性特征参数选取方法 总被引:3,自引:0,他引:3
为了评价地磁场特征参数对适配性的影响程度,达到选取重要特征参数目的,提出了一种基于粗糙集理论的地磁匹配制导适配性特征参数选取方法.通过分析粗糙集理论的基本原理,确定了特征参数选取的试验步骤;选取了适配性评价中具有代表性的6种特征参数作为条件属性集,在选定的28块区域基于积相关算法(PROD)进行了匹配仿真试验,选取匹配概率作为决策属性集,针对粗糙集理论只使用于离散数据的特点,分别对条件属性集和决策属性集进行了离散化处理;然后根据确定的试验步骤,对选定区域进行了特征参数选取试验,得到了约简特征参数集合,通过数据分析发现:提出的特征参数选取方法在不需要任何先验信息的情况下提取了约简特征参数集合,有效地排除了冗余信息的干扰,达到了选取重要特征参数的目的. 相似文献
5.
6.
叉流管-管型换热器二维温度场的数值分析 总被引:2,自引:0,他引:2
建立并导出叉流管-管型换热器传热过程的二维数学模型及相应的差分格式,对比实验数据和性能计算结果,表明数值方法是有效可行的。据此编制的计算机程序已成功地用于组合发动机空气预冷换热器工作过程的预测。 相似文献
7.
Zonal mean temperature, pressure, zonal wind and geopotential height as functions of latitude 总被引:8,自引:0,他引:8
Eric L. Fleming Sushil Chandra J. J. Barnett M. Corney 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1990,10(12):11-59
The new zonal mean COSPAR International Reference Atmosphere (CIRA-86) of temperature, zonal wind, and geopotential/geometric height is presented. This data can be used as a function of altitude or pressure and has nearly pole-to-pole coverage (80°S-80°N) extending from the ground to approximately 120 km. Data sources and methods of computation are described; in general, hydrostatic and thermal wind balance are maintained at all levels and latitudes. As shown by a series of cross sectional plots, the new CIRA accurately reproduces most of the characteristic features of the atmosphere such as the equatorial wind and the general structure of the tropopause, stratopause, and mesopause. 相似文献
8.
In part I (De Greve and Packet) we have investigated the occurrence of reversed phases of mass-transfer during Case A evolution in close binaries. If the initial period of a system is shorter than 1–2 days (Early Case A) the reversed phase starts before core hydrogen exhaustion of the gainer (part I). This type of evolution is characterized by at least two phases of slow mass-transfer.We have computed the evolution of four Early Case A systems with initial masses of the loser equal to 3 Mo and 5 Mo. These four systems start mass-exchange when Xc of the primary has decreased to 0.525 (75% of its initial value). They all experience two phases of slow mass-transfer.We find that both phases have about the same duration for all systems. The mass ratios are clearly distinct, being closer to unity during the first phase. In the Hertzsprung-Russell, mass-radius and mass-luminosity diagrams both components remain close to the main-sequence band during slow mass-transfer. Evolution as an Algol is ended when both components overflow their outer critical surface after a second reversal of the mass-transfer.Observed Algol systems evolving in Early Case A are scarce. A search thruogh the catalogue by Giuricin et al. gives us the following candidates: X Tri, SX Aur and V Pup. Based on their mass ratios, SX Aur can tentatively be assigned to the first phase of slow mass transfer and X Tri to the second phase. For V Pup (which is more massive) this choice can not be made with certainty. 相似文献
9.
10.
根据有关固体火箭发动机装药后端到喷管间的空间特征,对三维突扩后突缩内部流场计算进行了探索和研究。计算中成功地应用了SIMPLE算法解决复杂的三维流场计算问题,并在初场构成、源项离散及松弛系数的选取等方面都进行了调试改进。通过建立计算模型、划分网格、对方程及边界条件离散化和非线性处理,以及线性方程组求解等,计算得到了符合物理规律的数值解,指出了空间涡及二次涡的存在。 相似文献