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321.
322.
I.V. Arkhangelskaja A.I. Arkhangelsky E.V. Troitskaya L.I. Miroshnichenko 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
Accelerated energetic particles in solar flares produced nuclear γ-lines in interactions with ambient solar atmosphere. Analysis of intensity of ratios between various γ-lines allows us to make estimations of abundance of elements, parameters of surrounding media and other solar characteristics. In this article we discuss the flux ratio between two lines from excited states of 12C (f15.11/f4.44) and our results of preliminary calculation of intensity ratio between two neutron capture lines at 3He and 1H (f20.58/f2.223). In particular we consider the opportunity to obtain n(3He)/n(1H) ratio during solar flares and using high-energy gamma-emission studying, based on the satellite data. Possible interpretation of spectral features observed during the January 20, 2005 solar flare is discussed. Preliminary analysis of energy spectrum in the band of 2–21 MeV gives n(3He)/n(1H) ∼ 8 × 10−4 for January 20, 2005 solar flare. 相似文献
323.
P. Jovanović V. Borka Jovanović D. Borka T. Bogdanović 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
We used a model of a relativistic accretion disk around a supermassive black hole (SMBH), based on ray-tracing method in the Kerr metric, to study the variations of the composite Fe Kα line emitted from two accretion disks around SMBHs in a binary system. We assumed that the orbit of such a binary is approximately Keplerian, and simulated the composite line shapes for different orbital elements, accretion disk parameters and mass ratios of the components. The obtained results show that, if observed in the spectra of some SMBH binaries during their different orbital phases, such composite Fe Kα line profiles could be used to constrain the orbits and several properties of such SMBH binaries. 相似文献
324.
Hugh C. Pumphrey Richard E. Cofield Mark J. Filipiak Nathaniel J. Livesey 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
The Microwave Limb Sounder (MLS) instrument is a small satellite-borne radio telescope. Its purpose is to make limb-scanning measurements of atmospheric composition. One of the gases to which it is sensitive is carbon monoxide (CO), detected via the J = 2 → 1 rotational transition at 230 GHz. CO is present in molecular gas clouds in the Milky Way. Although it was not designed for the purpose, MLS can detect emissions from galactic CO, allowing a map of the 230 GHz radio sky to be constructed. We report the MLS measurements of galactic radio emission and discuss their effect on the atmospheric mission of MLS. The region of the Milky Way with emissions strong enough to significantly affect MLS observations of atmospheric CO is identified. Ground-based radio astronomers have been mapping the sky using CO emission for many years. However, the MLS data are the first such survey to be carried out from space. The MLS survey covers a larger area of the sky than any other 230 GHz survey, but no previously unknown gas clouds are observed. 相似文献
325.
按照国际民航组织规定的起飞着陆循环过程,简化飞机在机场起飞降落的活动路线,在原有飞机排放污染物排放指数(EI)计算的基础上,再结合飞机起飞降落过程的燃油流量(F),计算出进近、滑行、起飞、爬升四段路线的排放污染强度.基于高斯点源扩散公式,对其进行积分得线源扩散模型,再对线源扩散模型中的参数进行修正,建立了民航机场飞机排放浓度模型. 相似文献
326.
压电智能结构的实验研究 总被引:2,自引:0,他引:2
在复合材料表层铺设压电元件,利用压电元件能够实现力学量和电学量之间相互转化的独特性能,可将其用作传感器和驱动器,赋予材料和结构传感及动作的能力。本研究的压电材料采用锆钛酸铅压电陶瓷,基体材料采用玻璃纤维-环氧树脂复合材料,与外部信号采集和控制系统结合,构成了智能结构实验系统。本文对这一系统的损伤诊断和损伤主动控制功能进行了实验研究。该结构一方面可对冲击、过载等可能造成损伤的原因进行监测,并诊断裂缝、连接松动等损伤的产生和位置,另一方面还可自适应地驱动结构中的压电驱动器,改善结构应力状态,防止损伤的扩展。 相似文献
327.
为了探寻燃烧室进口空气温度、压力以及油气比对点熄火边界、温升、燃烧效率以及主要排放物摩尔分数的影响规律,
对航空发动机燃烧室在多工况下的点熄火特性、出口温度分布与主要排放物摩尔分数进行了试验测试。分别采用正癸烷的简化
反应机理与C 12 H 23 燃料的单步反应机理,对该燃烧室火焰筒内流场结构、温度场、中间组分与主要排放物摩尔分数分布特性进行了
数值计算,并与相应试验数据进行了对比分析。结果表明:随着燃烧室进口空气温度、压力以及油气比的提高,燃烧室燃烧效率、
温升、出口平均温度与NO X 摩尔分数逐渐提高,而UHC与CO摩尔分数逐渐降低;与采用C 12 H 23 燃料单步反应机理相比,采用正癸
烷的简化反应机理计算得到的火焰筒内流场与温度场分布更为合理,火焰筒出口温度场分布以及主要排放物摩尔分数与相应试
验数据更为接近,计算精度得到较大提高。 相似文献
328.
Adolfo L. Méndez Berhondo Ramón E. Rodríguez Taboada Paolo Zlobec Ana K. Díaz Rodríguez 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
Source length scales are estimated for the September 14, 2005 solar noise storm from the spectral and temporal observed characteristics of the background continuum fluctuations and clusters of Type I bursts. The characteristic height of the magnetic structure where the noise storm source is located and the size of the source where Type I bursts clustering takes place were calculated. A lower limit for the height of the magnetic structure supporting the noise storm at 237 MHz was estimated too. 相似文献
329.
从使用角度分析了靶试干扰机的特点。通过实例说明采用自卫式战术手段时,干扰掩护空域、干扰空间能量及干扰机发射功率、天线波束宽度的论证步骤与计算方法。给出了开关机、工作时间、可靠性、环境条件等参数值要求,并提出决策战技性能时应考虑的问题。 相似文献
330.