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261.
L. G. Blomberg J. A. Cumnock K.-H. Glassmeier R. A. Treumann 《Space Science Reviews》2007,132(2-4):575-591
The Hermean magnetosphere is likely to contain a number of wave phenomena. We briefly review what little is known so far about
fields and waves around Mercury. We further discuss a number of possible phenomena, including ULF pulsations, acceleration-related
radiation, bow shock waves, bremsstrahlung (or braking radiation), and synchrotron radiation. Finally, some predictions are
made as to the likelihood that some of these types of wave emission exist. 相似文献
262.
ANALYSISOFTHERETURNEDSIGNALMODELINBISTATICRADARSYSTEMSYinChengyou,XuShanjia,WangDongjin,ZhouLinyun(DepartmentofElectronicEngi... 相似文献
263.
Christian KlingenbergDepartment of Applied Mathematics Würzburg UniversityAm Hubland Würzburg Germany 《南京航空航天大学学报(英文版)》2001,18(Z1)
INTRODUCTIONConsider the Euler equations supplementedby an additional reactive equation which consistsof a scalar balance law for the mass fraction ofunburntgasρρuρEρY t+ρuρu2 + pρu E + upρu Y x=κ000-ρΘ( T) Ywhereρ is the density,ρu the momentum,ρEthe total specific energy,ρY the mass fraction ofunburnt gas( 0≤ Y≤ 1 ) ,κ a large number( thereaction rate) and T temperature.Θ( T) =01 if T≤ Tignif T>Tign,Tign is the ignition temperature,E=pγ- 1 + u22 + q0 Y,p is … 相似文献
264.
非正弦波大电流短辐射器设计研究 总被引:1,自引:1,他引:0
赫兹电偶极子是一种辐射非正弦波的短辐射器,对赫兹电偶极子而言,必须施加很高的驱动电压,才能得到较大的天线电流,从而导致其辐射功率往往很小.研究设计了一种大电流短辐射器,它具有馈电容易,结构简单且对称等优点,从而可以简化理论分析并便于工程应用. 相似文献
265.
本文应用一维混合模拟方法数值研究了准平行无碰撞激波的结构.结果表明,激波上游的质子和准平行无碰撞激波相互作用后,有部分质子被激波反射,并向激波上游运动很长一段距离,从而激发起束流不稳定性,引起大振幅的共振右旋偏振的低频波动.这些波动在太阳风的带动下向激波下游运动,靠近激波后与激波合井,同时在激波的上游不断有新的波动产生.此过程能不断重复地进行.在平行无碰撞激波的情况下,在激波的下游还有大振幅的非共振右旋偏振的低频波动.激波上游的低频波动在向下游运动的过程中强度不断加强,最后超过原来激波的强度,形成新的激波. 相似文献
266.
有涂覆层的导体圆柱空间散射特性的数值计算 总被引:1,自引:1,他引:0
黄兴中 《北京航空航天大学学报》1998,24(2):141-144
文中根据带有涂覆层的导体圆柱在平面波的照射下的散射场表达式,进行了全面的数值计算,说明了虚宗量的Bessel函数和Hankel函数的计算方法,分别给出了平行极化波和垂直极化波入射时双站RCS的计算曲线,包括不同涂覆层厚度的影响、入射波频率、涂覆层介质的相对介电常数、导磁率变化时双站RCS的变化规律,获得了有参考意义的结果. 相似文献
267.
G.S. Lakhina 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(10):1688-1694
Ion beams observed in the plasma sheet boundary layer (PSBL), cusp, and on the auroral zone field lines are expected to have spatial gradients in their drift velocity. Generation of kinetic Alfvén waves by velocity shear of the ion beams is discussed. It is shown that a hot ion beam can excite both a resonant kinetic Alfvén wave instability and a non-resonant coupled Alfvén-ion acoustic instability. For typical parameters, observed on the auroral field lines in the altitude range of 5–7 RE (where RE is the Earth’s radius), the frequency of the velocity shear modes, in the satellite frame of reference, lie in the ultra-low frequency (ULF) range. The noise due to velocity shear driven Alfvén modes is electromagnetic in nature, and has a finite parallel electric field component. 相似文献
268.
Sylvaine Turck-Chièze Suzanne Talon 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(6):855-860
The picture of the solar radiative zone is evolving quickly. This review is separated in two parts. We first recall how the two powerful probes of the solar interior, namely the neutrinos and helioseismology have scrutinized the microscopic properties of the solar radiative plasma. Recent observations stimulate today complementary activities beyond the standard stellar model through theoretical modeling of angular momentum transport by rotation, internal waves or (and) by magnetic fields to get access to the dynamical motions of this important region of the Sun. So in the second part, we summarize the first impact of such processes on the radiative zone. 相似文献
269.
A.P. Kakad S.V. Singh R.V. Reddy G.S. Lakhina S.G. Tagare 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009,43(12):1945-1949
Satellite observations have revealed solitary potential structures in the Earth’s magnetotail region. These structures have both positive (compressive) and negative (rarefactive) electrostatic potentials. In this paper we study the electron-acoustic solitary waves (EASWs) in an unmagnetized plasma consisting of cold plasma electrons and isothermal ions with two different temperatures. Using the reductive perturbation method, the nonlinear evolution of such structures is studied. The numerical computations are performed to study the role of two temperature ions in the generation of EASWs. In this case, the model supports the existence of both positive and negative electrostatic potentials with bipolar pulses. The electric field associated with these positive and negative solitary structures are numerically computed. The present study could be useful to construe the compressive and rarefactive electric field bipolar pulses associated with the BEN type emissions in the magnetospheric regions where the electron beams are not present. 相似文献
270.
A.K. Singh Rajesh Singh Kalpana Singh R.P. Singh 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(10):1695-1698
In this paper we report pulsing hiss emissions observed at the low latitude station, Jammu (geomag. lat. 22°26′N, L = 1.17) in which intensity decreases with the increase in frequency. The entire dynamic spectra contain somewhat irregular structure. To explain these we propose that the hiss emissions are generated through Doppler-shifted cyclotron interactions near the equator and propagate to the earth in the whistler-mode. Further, ULF waves present in the generation region modulate the intensity of the emission resulting in the pulsing nature. The growth rates are computed and discussed in the light of recent works. 相似文献