排序方式: 共有60条查询结果,搜索用时 156 毫秒
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可凝性气体对低温光学元件表面污染的测试设备 总被引:3,自引:0,他引:3
详细介绍了某些可凝性气体对低温光学元件表面污染测试设备的基本原理,基本结构及使用方法;对其主要性能进行了实验测定,并给出了系统误差分析,该设备结构简单,功能齐全,性能可靠,使用方便;测试波段从近红外直至远红外,精度优于3%,与国外同类仪器相当,可用于各类可凝性气冷凝霜层的测试研究,为进一步发展空间技术提供了有效的研究设备。 相似文献
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红外辐射大气透过率的工程计算 总被引:2,自引:0,他引:2
针对现有红外辐射大气透过率经验计算公式不适用于高层大气的局限性,对其进行了重新推导并引入了高度修正,修正后的公式可用于计算任意高度路程上的大气透过率,修正所需大气光学特性参数全部可查相关手册获得。此外,还设计了适合于计算倾斜路径上大气透过率的计算流程,并给出了计算实例。 相似文献
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Mai-Julie Nguyen François Raulin Patrice Coll Sylvie Derenne Cyril Szopa Guy Cernogora Guy Israël Jean-Michel Bernard 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
In the present work, we focused on the possible isotopic fractionation of carbon during the processes involved in the formation of Titan’s tholins. We present the first results obtained on the 12C/13C isotopic ratios measured on Titan’s tholins synthesized in laboratory with cold plasma discharges. Measurements of isotopic ratio 12C/13C, done both on tholins and on the initial gas mixture (N2:CH4 (98:2)) used to produce them, do not show any evident deficit or enrichment in 13C relatively to 12C in the synthesized tholins, compared to the initial gas mixture. This observation allows to go further in the analyses of the ACP experiment data, including part of the Cassini–Huygens mission. 相似文献
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K. Liu E. Kallio R. Jarvinen H. Lammer H.I.M. Lichtenegger Yu.N. Kulikov N. Terada T.L. Zhang P. Janhunen 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
As an initial effort to study the evolution of the Venus atmosphere, the influence of the solar wind density and the interplanetary magnetic field (IMF) x component (the x-axis points from Venus towards the Sun) on the O+ ion escape rate from Venus is investigated using a three-dimensional quasi-neutral hybrid (HYB-Venus) model. The HYB-Venus model is first applied to a case of the high-density (100 cm−3) solar wind interaction with Venus selected from the Pioneer Venus Orbiter observations to demonstrate its capability for the study. Two sets of simulations with a wide range of solar wind densities and different IMF x components are then performed. It is found that the O+ ion escape rate increases with increasing solar wind density. The O+ ion escape rate saturates when the solar wind density becomes high (above 100 cm−3). The results also suggest that the IMF x component enhances the O+ ion escape rate, given a fixed IMF component perpendicular to the x-axis. Finally, the results imply a higher ion loss rate for early-Venus, when solar conditions were dramatically different. 相似文献
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Model for induced ionization by galactic cosmic rays in the Earth atmosphere and ionosphere 总被引:1,自引:1,他引:0
P.I.Y. Velinov A. Mishev L. Mateev 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009,44(9):1002-1007
The ionization profiles produced by galactic cosmic rays in the Earth atmosphere and ionosphere are obtained on the basis of Monte Carlo simulations. Cascade processes in the atmosphere are simulated using CORSIKA 6.52 code with FLUKA 2006 and QGSJET II hadronic interaction subroutines. Proton induced showers are considered using a realistic atmospheric model (US Standard Atmosphere). The energy deposit from different components is taken into account, namely electromagnetic, hadron and muon components. The curvature of the atmosphere is considered in the computer code. On the basis of the computed ionization yield function the ion pair production rate in the atmosphere is obtained for different conditions and locations. The model is applicable to the entire atmosphere, from ground level to upper atmosphere. Several applications of the obtained results are discussed. The Monte Carlo simulation model considers nuclear interactions below the altitude of 35 km. It is compared with analytical–numerical electron production rate model. The latter model which takes into account the electromagnetic interactions above altitudes of 35 km has two main regions of application: above 50 km (thin target model) and between 35 and 50 km (intermediate target model). A good agreement between the CORSIKA results and analytical–numerical model results is found above altitude of 35 km. 相似文献
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A.A. Berezhnoy 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
The column densities of impact-produced metal atoms in the exosphere during the peaks of activity of the main meteor showers – Geminids, Quadrantids and Perseids – and during quiet periods are estimated. The Na supply rate is estimated to be 2 × 104, 3 × 103, 104, and 2 × 104 atoms cm−2 s−1 for sporadic meteoroids, Perseid, Geminid, and Quadrantid meteor showers, respectively. A low upper limit on Ca in the lunar exosphere is explained by the condensation of Ca into dust grains during expansion of the cooling impact-produced vapor cloud. The chemical composition of gas-phase species released to the lunar exosphere during meteoroid impacts has been estimated. Most impact-produced molecules that contain metals are destroyed by solar photons while on ballistic trajectories. Energies of Na, K, Ca, and Mg atoms produced via photolysis of the respective monoxides are estimated to be 0.4, 0.35, 0.6, and 0.45 eV, respectively. The relative content of impact-produced Na and K atoms is maximal at altitudes of about 1000–2000 km and during the main meteor showers, lunar eclipses, and passages of the Moon through the Earth’s magnetosphere. 相似文献
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空气环境质量状况模糊综合评价分析 总被引:2,自引:0,他引:2
通过利用模糊综合评价方法对某地区的空气环境质量监测数据状况进行分析与评价,并考虑到各种对环境质量影响,经综合模糊性和随机性分析证明:模糊综合评价方法简单,结论客观地反映了某地区的空气环境质量水平,与实际的空气污染现状相符. 相似文献
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