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1.
高精度CTD剖面仪电导率传感器的研究和实验 总被引:3,自引:2,他引:3
高精度CTD剖面仪是海洋863项目的重要组成部分,是海洋调查和水文观测必不可少的仪器,本文详细论述了CTD剖面仪中电导率传感器的研制方法和过程,并给出传感器现已达到的水平,提出还需要进一步进行的工作和深入研究的问题。 相似文献
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本文介绍了2000Mc太阳射电望远镜本机振荡器改造的基本原理,以及本机振荡器的主要技术指标进行检测的结果,结果表明主要技术参数达到了原设计指标。 相似文献
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介绍了一种采用锁相环技术(PLL)产生高稳定度正弦信号的宽频带频率合成器方案,在该系统中采用锁相环频率合成器芯片ADF4360-7设计锁相环电路.简要分析了该芯片的工作原理,并给出了频率合成器的电路参数.通过该系统实现的宽频带本振信号的输出频率范围达到500 MHz~1 GHz. 相似文献
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Using a non-local and time-dependent theory of convection, we have cal- culated the linear non-adiabatic oscillations of the radial and low-degree F-p39 modes for evolutionary models from the main sequence to the asymptotic giant branch for stars with solar abundance (X = 0.70, Z = 0.02) in the mass range of 0.6-3.0 3//o. The results show that iow luminosity cool stars tend to be solar-like oscillators, whose low-order modes are stable, but intermediate and high order p-modes are pulsationally unstable; their unstable modes have a wide range in frequency and small values for amplitude growth rates. For stars with increasing luminosity and therefore lower tem- perature, the unstable modes shift towards lower orders, the corresponding range of frequency decreases, and the amplitude growth rate increases. High luminosity red gi- ant stars behave like typical Mira-like oscillators. The effects of the coupling between convection and oscillations on pulsational instability have been carefully analyzed in this work. Our research shows that convection does not simply act as a damping mechanism for oscillations, and the complex nature of the coupling between convec- tion and oscillations makes turbulent convection sometimes behave as damping, and sometimes as excitation. Such a picture can not only naturally account for the red edge of the instability strip, but also the solar-like oscillations in low luminosity red stars and Mira-like ones in high luminosity red giants. 相似文献
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本文介绍了青海站137米射电望远镜上3mm振荡器恒温电路的改进情况。新的恒温电路有别于原来所使用的恒温电路的工作方式。实际使用证明,该电路性能可靠,显著提高了系统稳定性。 相似文献
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介绍了一种仅用销模Nd:YAG振荡器进行的卫星激光测距实验。此类振荡器的倍频输出可达5-10mJ(532nm),脉宽50-100ps。整个振荡器仅采用一支氙灯和一支Nd:YAG棒,体积紧凑、小巧,重量仅32kg。接收望远镜口径为60cm,单光子雪崩二极管接收器。本系统对8000km远的Lageos-1,Lageos-2两颗卫星进行了成功的测距。 相似文献
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A class of E1 Niйo atmospheric physics oscillation model is considered. The E1 Niйo atmospheric physics oscillation is an abnormal phenomenon involved in the tropical Pacific ocean-atmosphere interactions. The conceptual oscillator model should consider the variations of both the eastern and western Pacific anomaly patterns. An E1 Niйo atmospheric physics model is proposed using a method for the variational iteration theory. Using the variational iteration method, the approximate expansions of the solution of corresponding problem are constructed. That is, firstly, introducing a set of functional and accounting their variationals, the Lagrange multiplicators are counted, and then the variational iteration is defined, finally, the approximate solution is obtained. From approximate expansions of the solution, the zonal sea surface temperature anomaly in the equatorial eastern Pacific and the thermocline depth anomaly of the sea-air oscillation for E1 Niйo atmospheric physics model can be analyzed. E1 Niйo is a very complicated natural phenomenon. Hence basic models need to be reduced for the sea-air oscillator and are solved. The variational iteration is a simple and valid approximate method. 相似文献