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151.
功率控制对于允许次用户和主用户之间频谱共享的认知无线电网络来说是关键的,针对具有干扰限制的认知网络最大总容量得到一种最优的分步式功率控制策略,对于系统效用的非凸性,引入几何规划把非凸最优化问题转换为凸最优化问题,引入辅助变量和额外等式约束,把效用之间的关联转化为约束之间的关联,提出了功率控制策略的解决方法,显示了整体最... 相似文献
152.
Katinka Geréb Sándor Frey 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The point source list of the Wilkinson Microwave Anisotropy Probe (WMAP) is a uniform, all-sky catalogue of bright sources with flux density measurements at high (up to 94 GHz) radio frequencies. We investigated the five-year WMAP list to compile a new catalogue of bright and compact extragalactic radio sources to be potentially studied with Very Long Baseline Interferometry at millimeter wavelengths (mm-VLBI) and Space VLBI (SVLBI). After comparing the WMAP data with the existing mm-VLBI catalogues, we sorted out the yet unexplored sources. Using the 41, 61 and 94 GHz WMAP flux densities, we calculated the spectral indices. By collecting optical identifications, lower-frequency radio flux densities and VLBI images from the literature, we created a list of objects which have not been investigated with VLBI at 86 GHz before. With total flux density at least 1 Jy and declination above −40°, we found 37 suitable new targets. It is a nearly 25% addition to the known mm-VLBI sources. Such objects are also potentially useful as phase-reference calibrators for the future Japanese SVLBI mission ASTRO-G at its highest observing frequency (43 GHz). The phase-referencing capability of ASTRO-G would allow long integrations and hence better sensitivity for observing faint target sources close to suitable phase calibrators in the sky. 相似文献
153.
G. P. Chernov 《Space Science Reviews》2006,127(1-4):195-326
This review covers fairly comprehensively experimental and theoretical research on the fine structure of types zebra pattern
(ZP) and fiber bursts (FB) in solar type II + IV radio bursts. The basic attention is given to the latest experimental data.
A comparative analysis of several recent solar type IV radio outbursts with these fine structure in dynamical radio spectra
is carried out using available ground-based and satellite data (Yohkoh, SOHO, TRACE, RHESSI). New data on microwave zebra
structures and fiber bursts testifies that they are analogous to similar structures observed at meter wavelengths. The discovery
of the superfine structure, in the form of millisecond spikes is the most significant new effect in the cm range. All basic
theoretical models of the zebra pattern and fiber bursts are discussed critically. Two main models are studied for their interpretation:
(i) interactions between electrostatic plasma waves and whistlers, (ii) radio emission at double plasma resonance (DPR). The
relative significance of several possible mechanisms remains uncertain. 相似文献
154.
155.
Jeongwoo Lee 《Space Science Reviews》2007,133(1-4):73-102
Solar active region coronae are known for strong magnetic fields permeating tenuous plasma, which makes them an ideal astronomical
laboratory for magnetohydrodynamics research. It is, however, relatively less known that this physical condition also permits
a very efficient radiation mechanism, gyro-resonant emission, produced by hot electrons gyrating in the coronal magnetic field.
As a resonant mechanism, gyro-emission produces high enough opacity to fully reveal the coronal temperature, and is concentrated
at a few harmonics of the local gyrofrequency to serve as an excellent indicator of the magnetic field. In addition, the polarization
of the ubiquitous free–free emission and a phenomenon of depolarization due to mode coupling extend the magnetic field diagnostic
to a wide range of coronal heights. The ability to measure the coronal temperature and magnetic field without the complications
that arise in other radiative inversion problems is a particular advantage for the active region radio emissions available
only at these wavelengths. This article reviews the efforts to understand these radiative processes, and use them as diagnostic
tools to address a number of critical issues involved with active regions. 相似文献
156.
软件接收机中内部自动增益控制的DSP实现 总被引:1,自引:0,他引:1
本文给出了软件接收机中内部自动增益控制(AGC)的一种算法,该算法运算量小、适于DSP采用。文中最后给出算法的仿真结果。 相似文献
157.
研究多功能可重构软件无线电开发、测试与评估通用平台技术,验证多信道软件无线电技术可实现性,突破平台设备实现级关键技术,通过论证,证明了基于通用平台的测试及故障诊断技术的可行性,及多信道软件无线电在不同应用领域通信系统的适应性和可重构性。 相似文献
158.
159.
T.L. Gulyaeva 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(5):1588-1595
The international reference ionosphere, IRI, and its extension to plasmasphere, IRI-Plas, models require reliable prediction of solar and ionospheric proxy indices of solar activity for nowcasting and forecasting of the ionosphere parameters. It is shown that IRI prediction errors could increase for the F2 layer critical frequency foF2 and the peak height hmF2 due to erroneous predictions of the ionospheric global IG index and the international sunspot number SSN1 index on which IRI and IRI-Plas models are built. Regression relation is introduced to produce daily SSN1 proxy index from new time series SSN2 index provided from June 2015, after recalibration of sunspots data. To avoid extra errors of the ionosphere model a new solar activity prediction (SAP) model for the ascending part of the solar cycle SC25 is proposed which expresses analytically the SSN1 proxy index and the 10.7-cm radio flux F10.7 index in terms of the phase of the solar cycle, Φ. SAP model is based on monthly indices observed during the descending part of SC24 complemented with forecast of time and amplitude for SC25 peak. The strength of SC25 is predicted to be less than that of SC24 as shown with their amplitudes for eight types of indices driving IRI-Plas model. 相似文献
160.
提出一种基于简化Volterra级数模型的射频接收机电磁敏感性(EMS,Elec-tromagnetic Susceptibility)行为级仿真方法.利用3阶简化Volterra级数模型对接收机EMS进行分析,根据EMS频响特性,提出一种通用的EMS判据,并给出敏感度阈值仿真求解流程图.弥补了以往在接收机EMS分析时以试验为主,缺乏仿真分析的缺陷.以某双频GPS(GlobalPositioning System)接收机受连续波干扰为例,对带内和带外(包括镜频和互调)敏感度阈值进行求解.仿真结果表明该方法不仅有效、可行,而且减少了敏感度阈值求解所需的内存空间和仿真运行时间,适应于一般射频接收机的EMS分析,在工程技术领域切合实际. 相似文献