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81.
82.
T. Sindelarova D. BuresovaJ. Chum F. Hruska 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
Ionospheric effects of meteorological origin observed by the continuous HF Doppler sounder over the Czech Republic are reported in this paper. We focused on detection of waves of periods 1–10 min. We discuss the influence of dynamics and intensity of active weather systems on the occurrence of short period waves and dependence of the observed ionospheric effects on the height of reflection of the sounding radio wave. We observed 3–5 min waves during a severe weather event in summer and 2.5–4 min waves during a severe weather event in winter. We excluded possible geomagnetic origin of these oscillations by the analysis of fluctuations of the local geomagnetic field. In eight cases of 10, wave activity in the analysed period range was not significantly increased comparing to quiet days. The intensity of weather systems as well as the location of potential sources of waves towards the points of HF Doppler shift observation influence significantly the occurrence of infrasonic waves in the ionosphere. The results in Central Europe differ considerably from those previously obtained in North America. As a possible reason, we discuss different intensity and dynamics of weather systems in both regions. 相似文献
83.
V.B. Baranov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
An interface between the fully ionized hydrogen plasma of the solar wind (SW) and the partially ionized hydrogen gas flow of the local interstellar medium (LISM) is formed as a region where there is a strong interaction between these two flows. The interface is bounded by the solar wind termination shock (TS) and the LISM bow shock (BS) and is separated on two regions by the heliopause (HP) separating the solar wind and charged component of the LISM (plasma component below). The BS is formed due to the deceleration of the supersonic LISM flow relative to the solar system. Regions of the interface between the TS and HP and between the HP and BS were in literature named as the inner and outer heliosheaths, respectively. An investigation of the structure and physical properties of the heliosheath is at present especially interested due to the fact that Voyager-1 and Voyager-2 have crossed the TS in December 2004 (Burlaga, L.F., Ness, N.F., Acuna, M.Y., et al. Crossing the termination shock into the the heliosheath. Magnetic fields. Science 309, 2027–2029, 2005; Fisk, L.A. Journey into the unknown beyond. Science 309, 2016–2017, 2005; Decker, R.B., Krimigis, S.M., Roelof, E.C., et al. Voyager 1 in the foreshock, termination shock and heliosheath. Science 309, 2020–2024, 2005; Stone, E.C., Cummings, A.C., McDonald, F.B., et al. Voyager 1 explores the termination shock region and the heliosheath beyond. Science 309, 2017–2020, 2005) and in September 2007 (Jokipii, J.R. A shock for Voyager 2. Nature 454, 38–39, 2008; Gurnett, D.A., Kurth, W.S. Intense plasma waves at and near the solar wind termination shock. Nature 454, 78–80, 2008. doi: 10.1038/nature07023; Wang, L., Lin, R.P., Larson, D.E., Luhmann, J.G. Domination of heliosheath pressure by shock-accelerated pickup ions from observations of neutral atoms. Nature 454, 81–83, 2008. doi: 10.1038/nature07068.14; Burlaga, L.F., Ness, N.F., Acuna, M.H., et al. Magnetic fields at the solar wind termination shock. Nature 454, 75–77, 2008. doi: 10.1038/nature07029; Richardson, J.D., Kasper, J.C., Wang, C., et al. Cool heliosheath plasma and deceleration of the upstream solar wind at the termination shock. Nature 454, 63–66, 2008. doi: 10.1038/nature07024; Stone, E.C., Cummings, A.C., McDonald, F.B., et al. An asymmetric solar wind termination shock. Nature 454, 71–74, 2008. doi: 10.1038/nature07022; Decker, R.B., Krimigis, S.M., Roelof, E.C., et al. Mediation of the solar wind termination shock by non-thermal ions. Nature 454, 67–70, 2008. doi: 10.1038/nature 07030), respectively, and entered to the inner heliosheath. 相似文献
84.
大攻角条件下的二维进气道型面优化设计 总被引:1,自引:0,他引:1
基于一维气体动力学,以进气道前体楔面楔角为优化设计参数,以总压恢复系数、流量系数最大及阻力系数最小为优化目标,对二维进气道外型面进行了优化设计,并综合考虑了大攻角条件下的位于背风面与迎风面上进气道面临的不同来流条件.在优化设计中,采用改进后的NSGA-Ⅱ遗传算法.在问题求解中,对NSGA-Ⅱ算法的交叉算子及优选策略进行了改进.优化结果表明.总压恢复系数与阻力系数的优化结果具有一致性,即二者可同时达到最优;第一级楔角的大小对流量系数的影响显著.对优化结果进行了数值模拟,数值模拟结果表明,文中设计的型面构型满足设计要求.该设计方法可用于二维进气道型面考虑攻角条件下的初步设计. 相似文献
85.
图像压缩的基础在于图像数据存在信息的冗余性,而对图像模糊的变换能够增加图像的信息冗余,为此提出在传统图像压缩方法中引入模糊变换环节,以增加图像压缩比。实验结果表明,引入模糊变换后能有效提高图像的压缩比。 相似文献
86.
Dong L. Wu Michael J. Schwartz Joe W. Waters Varavut Limpasuvan Qian Wu Timothy L. Killeen 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
This paper describes a microwave limb technique for measuring Doppler wind in the Earth’s mesosphere. The research algorithm has been applied to Aura Microwave Limb Sounder (MLS) 118.75 GHz measurements where the O2 Zeeman lines are resolved by a digital autocorrelation spectrometer. A precision of ∼17 m/s for the line-of-sight (LOS) wind is achieved at 80–92 km, which corresponds to radiometric noise during 1/6 s integration time. The LOS winds from Aura MLS are mostly in the meridional direction at low- and mid-latitudes with vertical resolution of ∼8 km. This microwave Doppler technique has potential to obtain useful winds down to ∼40 km of the Earth’s atmosphere if measurements from other MLS frequencies (near H2O, O3, and CO lines) are used. Initial analyses show that the MLS winds from the 118.75 GHz measurements agree well with the TIDI (Thermosphere Ionosphere Mesosphere Energetics and Dynamics Doppler Interferometer) winds for the perturbations induced by a strong quasi 2-day wave (QTDW) in January 2005. Time series of MLS winds reveal many interesting climatological and planetary wave features, including the diurnal, semidiurnal tides, and the QTDW. Interactions between the tides and the QTDW are clearly evident, indicating possible large tidal structural changes after the QTDW events dissipate. 相似文献
87.
Katia Ferrière 《Space Science Reviews》2006,122(1-4):247-253
We present a theoretical overview of low-frequency waves and instabilities in collisionless, multi-component plasmas with
gyrotropic (
) thermal pressure. We show that the complete dispersion relation can be obtained in the framework of a mixed magnetohydrodynamic
(MHD)-kinetic formalism, which uses the MHD mass, momentum, and induction equations, together with the kinetically corrected
version of the double-adiabatic equations of state. The complete dispersion relation contains not only the three standard
modes (fast, slow, and Alfvén) from double-adiabatic MHD, but also the mirror mode from kinetic theory. We examine the stability
properties of these four modes, firstly in the case of a uniform medium, and secondly in the case of a stratified and rotating
medium. We also discuss the connections with the quasi-interchange modes (interchange and translation) often referred to in
the context of magnetospheric physics. 相似文献
88.
89.
分析内爆炸圆管膨胀破碎过程的应力,提出确定内爆炸圆管断裂半径的复合判据,从理论上预测不同材料圆管的破片初速度.采用GSJ高速摄影记录仪测试不同材料圆管的破片初速度,并与理论预测值行比较.结果表明,采用复合判据得到的理论预测结果与实验测量结果能够较好吻合. 相似文献
90.
面向航天器编队飞行的需求,对椭圆参考轨道航天器非线性周期相对运动条件进行研究,提出了确定椭圆参考轨道编队航天器非线性周期性相对运动条件的新方法。首先,考虑非线性、椭圆轨道等因素,通过哈密尔顿-雅可比(HJ)方程和正则摄动理论,推导了在任意非线性摄动下相对运动的模型和获得不需消耗任何燃料的周期性相对运动轨道的条件;然后,采用时域配点法,结合改进的列文伯格-马夸尔特(LM)法对周期性相对运动的初值进行求解;最后,设计数值仿真算例,利用上述条件,得到不消耗任何燃料的周期性绕飞轨道,由此验证了本文所提模型和方法的正确性。 相似文献