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1.
弹载引信电控扫描识别目标方位的方法 总被引:1,自引:0,他引:1
研究了弹载引信电控扫描识别目标方位的一种方法,该方法是:首先研究一种周期电控脉冲起动单刀四掷微波开关,该开关又逐次起动可瞄准定向天线的每一元和它们的公共收发系统。因而该系统既能全向搜索空中目标,又能分区截取回波信号,由此获得引信天线电控扫瞄形式的可瞄准探测系统。 相似文献
2.
小直径刀具(φ6mm以下小钻头、铣刀)加工中产生的磨、破损信号难于检测。本文基于这一问题,研究采用无线电遥测技术来传输传感器信号,并建立了CIMS,FMS加工中心钻、铣用小直径刀具的工况监视系统。研究表明:用遥测技术传输的切削过程信息是可以用来识别刀具切削状态的;小直径刀具折断快速报警的成功率在90%以上。 相似文献
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D. B. Melrose 《Space Science Reviews》1994,68(1-4):159-170
The theory of electron cyclotron maser emission and its application to solar spike bursts are reviewed. By analogy with the Earth's AKR, three sources of free energy are considered: a loss-cone anisotropy, a velocity-space hole, and a trapped distribution. The problem of how the radiation escapes through the second harmonic absorption layer is emphasized. Harmonic emission due to z mode coalescence may operate for some bursts, but the 2–5s delay between hard X-ray bursts and spike bursts suggests that some other mechanisms is required for most spike bursts. A model involving formation of a trapped distribution in low-density regions neighboring the flaring flux tube is considered. 相似文献
5.
We present models of the extragalactic background light (EBL) based on several scenarios of galaxy formation and evolution. We have treated galaxy formation with the Press-Schecter approximation for both cold dark matter (CDM) and cold+hot dark matter (CHDM) models, representing a moderate (z
f
3) and a late (z
f
1) era of galaxy formation respectively. Galaxy evolution has been treated by considering a variety of stellar types, different initial mass functions and star formation histories, and with an accounting of dust absorption and emission. We find that the dominant factor influencing the EBL is the epoch of galaxy formation. A recently proposed method for observing the EBL utilizing the absorption of 0.1 to 10 TeV gamma-rays from active galactic nuclei (AGN) is shown to be capable of discriminating between different galaxy formation epochs. The one AGN viewed in TeV light, Mrk 421, does show some evidence for a cutoff above 3 TeV; based on the EBL models presented here, we suggest that this is due to extinction in the source. The large absorption predicted at energies > 200 GeV for sources at z > 0.5 indicates that observations of TeV gamma-ray bursts (GRB) would constrain or eliminate models in which the GRB sources lie at cosmological distances.Now at University of Chicago, Dept. of Astronomy & Astrophysics. 相似文献
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F.B. Rizzato A.C.-L. Chian M.V. Alves R. Erichsen S.R. Lopes G.I. de Oliveira R. Pakter E.L. Rempel 《Space Science Reviews》2003,107(1-2):507-514
Langmuir waves and turbulence resulting from an electron beam-plasma instability play a fundamental role in the generation
of solar radio bursts. We report recent theoretical advances in nonlinear dynamics of Langmuir waves. First, starting from
the generalized Zakharov equations, we study the parametric excitation of solar radio bursts at the fundamental plasma frequency
driven by a pair of oppositely propagating Langmuir waves with different wave amplitudes. Next, we briefly discuss the emergence
of chaos in the Zakharov equations. We point out that chaos can lead to turbulence in the source regions of solar radio emissions.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
8.
Several examples of the radio emission of eruptive solar flares with high-frequency slowly drifting structures and type II
bursts are presented. Relationships of these radio bursts with eruptive phenomena such as soft X-ray plasmoid ejection and
shock formation are shown. Possible underlying physical processes are discussed in the framework of the plasmoid ejection
model of eruptive solar flares. On the other hand, it is shown that these radio bursts can be considered as radio signatures
of eruptive solar flares and thus used for the prediction of heliospheric effects.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
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10.
Noise in wireless systems from solar radio bursts 总被引:1,自引:0,他引:1
L.J. Lanzerotti D.E. Gary G.M. Nita D.J. Thomson C.G. Maclennan 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2005,36(12):2253-2257
Solar radio bursts were first discovered as result of their interference in early defensive radar systems during the Second World War (1942). Such bursts can still affect radar systems, as well as new wireless technologies. We have investigated a forty-year record of solar radio burst data (1960–1999) as well as several individual radio events in the 23rd solar cycle. This paper reviews the results of a portion of this research. Statistically, for frequencies f 1 GHz (near current wireless bands), there can be a burst with amplitudes >103 solar flux units (SFU; 1 SFU = 10−22 W/m2) every few days during solar maximum conditions, and such burst levels can produce problems in contemporary wireless systems. 相似文献