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1.
Zhaohui Shang Beverley J. Wills Edward L. Robinson 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,34(12):2579-2583
We have performed a spectral principal component analysis for a complete sample of 22 low redshift QSOs with spectra from Ly to H, and found three significant principal components, which account for 78% of the spectrum-to-spectrum variance. We present strong arguments that the first principal component represents the Baldwin effect, relating equivalent widths to the luminosity (i.e. accretion rate). The second component represents continuum variations, probably dominated by intrinsic reddening. The third principal component is directly related to broad emission-line width and X-ray spectral index, and therefore probably driven by Eddington accretion ratio, L/LEdd. The third set of relationships tie directly to the optical Principal Component 1 found by Boroson and Green [Boroson, T., Green, R.F., Astrophys. J. Suppl. 80, 109, 1992 (BG92)], and are the primary cause of scatter in the Baldwin relationships. 相似文献
2.
Magnetic reconnection is a universal phenomenon where energy is efficiently converted from the magnetic field to charged particles
as a result of global magnetic topology changes during which earlier separated plasma regions become magnetically connected.
While the reconnection affects large volumes in space most of the topology changes and of the energization occur within small
localized regions. Regions of special importance are the X-region and the separatrix region. The understanding of the microphysics
of these regions is crucial for the overall understanding of the reconnection. The Earth magnetosphere is the best environment
where the details of these regions can be studied in situ. We summarize their main properties and discuss recent spacecraft observations. 相似文献
3.
K. Fayazbakhsh A. Abedian 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
Using low power electronic devices for space applications to reduce the mass and energy consumption has lead to electromagnetic interference (EMI) problem. Electronic enclosures are used to shield electronic devices against EMI. In the past, electromagnetic shielding has been mainly the only criteria considered in electronic enclosure design. However, there are several structural and thermal requirements for selection of shielding materials which should also be taken into account. In this research work, three quantitative materials selection methods, i.e. Digital Logic (DL), Modified Digital Logic (MDL), and Z-transformation, are employed to select the best material from among a list of candidate materials. Composite and metallic electronic enclosures are explored and the best material is selected. Z-transformation method is applicable to both of the considered case studies while DL and MDL can only be used for solving one of them. Z-transformation method ranks aluminum as the first choice among various metallic materials. The wide range of Z-transformation application and its practical results confirm the superiority of Z-transformation method over DL and MDL methods. 相似文献
4.
丁小云 《西安航空技术高等专科学校学报》2014,(4):34-38
我国经济高速发展,劳动力、土地等要素随之发生转变,加工贸易从东部地区向中西部地区转移,中西部地区加工贸易急需升级以适应发展。利用2001-2011年中西部地区部分省份的面板数据建立计量模型,通过检验对混合估计模型、固定效应模型和随机效应模型进行选择,并对选定模型的估计结果进行具体分析,提出中西部地区加工贸易升级的对策及建议。 相似文献
5.
介绍了一种应用于人工辅助心脏的永磁轴承无位置传感器盘式无刷直流电动机的结构与电磁场仿真计算方法及结果,并对其温度场进行仿真计算。该电机体积重量小,无机械轴承,避免了对血液的破坏,且运行安全可靠。 相似文献
6.
火星稀薄的大气使得探测器再入火星时难以获得足够的减速阻力,为此,文章提出利用磁阻尼增加阻力的概念。高速再入的探测器与火星大气剧烈摩擦产生等离子体,利用探测器上的磁偶极场将等离子体捕获,同时在火星大气中形成一个“磁泡”区域并跟随探测器。由“磁泡”束缚的等离子体与来流的中性气体发生碰撞获得动量,又通过磁场作用将动量传递给探测器,从而使探测器获得一定的减速阻力。在磁阻尼的作用下,在同样的开伞高度探测器速度可降至更低,而低速开伞又可提高阻力伞打开的可靠性。因此,磁阻尼不仅可加快降低再入速度,而且还有助于提高探测器着陆火星的安全性。 相似文献
7.
提出了一种利用辅助信息消除多普勒频移、减小子载波间干扰(ICI)、降低误码率的方法,即信息辅助抗多普勒频移方法(IAADO)。飞机利用自身配置的导航系统、监视等多种信息系统,可以实时或准实时地获得自身和周围飞机及地面站的位置、运动状态等信息,从而计算出接收信号的多普勒频移,并在此基础上采取频率补偿措施来消除多普勒频移在OFDM系统中产生的ICI。仿真结果表明,基于辅助信息的IAADO方法有效地解决了航空宽带移动通信中多普勒效应造成的强ICI干扰问题,提高了高速移动航路环境下的通信性能,IAADO和信道估计(导频点LS估计、线性插值)的联合使用可以进一步增强终端区环境下的通信性能。 相似文献
8.
A. G. Yahnin I. V. Despirak A. A. Lubchich B. V. Kozelov N. P. Dmitrieva M. A. Shukhtina H. K Biernat 《Space Science Reviews》2006,122(1-4):97-106
Although the auroral substorm has been long regarded as a manifestation of the magnetospheric substorm, a direct relation
of active auroras to certain magnetospheric processes is still debatable. To investigate the relationship, we combine the
data of the UV imager onboard the Polar satellite with plasma and magnetic field measurements by the Geotail spacecraft. The
poleward edge of the auroral bulge, as determined from the images obtained at the LHBL passband, is found to be conjugated
with the region where the oppositely directed fast plasma flows observed in the near-Earth plasma sheet during substorms are
generated. We conclude that the auroras forming the bulge are due to the near-Earth reconnection process. This implies that
the magnetic flux through the auroral bulge is equal to the flux dissipated in the magnetotail during the substorm. Comparison
of the magnetic flux through the auroral bulge with the magnetic flux accumulated in the tail lobe during the growth phase
shows that these parameters have the comparable values. This is a clear evidence of the loading–unloading scheme of substorm
development. It is shown that the area of the auroral bulge developing during substorm is proportional to the total (magnetic
plus plasma) pressure decrease in the magnetotail. These findings stress the importance of auroral bulge observations for
monitoring of substorm intensity in terms of the magnetic flux and energy dissipation. 相似文献
9.
本文分析了X-114型地效飞机的纵向气动布局的主要特点,即平底机翼翼型,倒三角平面形状,低置前外翼和高置大容量平尾,根据这些特点,说明X-114型地效飞机是如何获得纵向稳定性(包括俯稳定性和飞高稳定性)的。 相似文献
10.
Yihua Yan 《Space Science Reviews》2005,121(1-4):213-221
The coronal magnetic field configuration is important for understanding the energy storage and release processes that account
for flares and/or CMEs. Here we present a model which is based on the work for potential magnetic field problems that only
applies the condition at infinity with the boundary condition on the solar surface specified. We also discuss some recent
progress on general force-free field models. For some event analyses, we have employed MDI/SOHO longitudinal magnetogram insected
into the synoptic magnetogram to obtain whole boundary condition over the solar surface. Globally, the extrapolated global
magnetic field structures effectively demonstrate the case for the disk signature of the radio CMEs and the evolution of the
radio sources during the CME/flare processes. 相似文献