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981.
In this paper we continue the analysis of the influence of solar and interplanetary events on magnetic storms of the Earth that was started in [9, 10]. Different experimental results on solar-terrestrial physics are analyzed in the study and the effects are determined that arise due to differences in the methods used to analyze the data. The classifications of magnetic storms by the K
p and D
st indices, the solar flare classifications by optical and X-ray observations, and the classifications of different geoeffective interplanetary events are compared and discussed. It is demonstrated that quantitative estimations of the relationships between two types of events often depend on the direction in which the events are compared. In particular, it was demonstrated that the geoeffectiveness of halo CMEs (that is, the percentage of Earth-directed coronal mass ejections that result in geomagnetic storms) is 40–50%. Higher values given in some papers were obtained by another method, in which they were defined as the probability of finding candidates for a source of geomagnetic storms among CMEs, and, strictly speaking, these values are not true estimates of the geoeffectiveness. The latter results are also in contrast with the results of the two-stage tracing of the events: first a storm—an interplanetary disturbance, and then an interplanetary disturbance—a CME. 相似文献
982.
983.
固体火箭发动机性能精度分析 总被引:1,自引:2,他引:1
根据固体火箭发动机内弹道计算模型,提出了内弹道计算中的独立随机变量,建立了随机变量的概率统计模型,确定了参数的分布规律,并用Monte—Carlo法进行了内弹道模拟计算。最后对发动机性能的均值。和标准差σ进行了分析和实验验证,得出了计算方法可行,数据可信的结论。 相似文献
984.
为了克服在复合团体推进剂浇注过程中采用的常规真空浇注工艺的缺陷,采用了振动浇注技术。对6种配方的高粘度丁羟推进剂进行了实验研究,得出了适用的振动频率和加速度范围。该浇注技术已应用于某小型发动机装药生产中,成品合格率达100%。 相似文献
985.
E. V. Babkin M. Yu. Belyaev N. I. Efimov V. V. Sazonov V. M. Stazhkov 《Cosmic Research》2001,39(1):23-37
The results of determining the rotational motion of the Mir orbital station are presented for four long segments of its unmanned uncontrolled flight in 1999–2000. The determination was carried out using the data of onboard measurements of the Earth's magnetic field intensity. These data, taken for a time interval of several hours, were jointly processed by the least squares method with the help of integration of the equations of station motion relative to its center of mass. As a result of this processing, the initial conditions of motion and the parameters of the mathematical model used were evaluated. The technique of processing is verified using the telemetry data on angular velocity of the station and its attitude parameters. Two types of motion were applied on the investigated segments. One of them (three segments) presents a rotation around the axis of the minimum moment of inertia. This axis executes small oscillations with respect to a normal to the orbit plane. Such a motion was used for the first time on domestic manned orbital complexes. The second type of motion begins with a biaxial rotation which, in a few weeks, goes over into a motion very similar to the rotation around the normal to the orbit plane, but around the axis of the maximum moment of inertia. 相似文献
986.
基于参数估计的故障诊断方法因为具有确定故障发生的时间、位置和程度的能力而越来越引起人们的重视。时变(快速的或慢速的)参数辨识是基于参数估计故障诊断方法的关键。本文根据系统的变化,基于模糊控制的原理自动调整遗忘因子,导出了一种实现比较简单,对参数的时变具有较高跟踪速度和跟踪精度的辨识方法。理论分析和仿真试验证实了该方法的有效性 相似文献
987.
本文介绍一种遥感相机自动调焦技术的实验研究结果,实验表明,差分式对比传递函数法调焦,具有调焦精度高,调焦速度快,受像移影响不明显,适应性好等优点。 相似文献
988.
989.
丁羟推进剂粘接体系中的组分迁移 总被引:3,自引:1,他引:3
用浸泡增重法研究了衬层、绝热层对DOS和T27的吸收能力,用气相色谱仪研究了HTPB推进剂/HTPB衬层/EPDM绝热层粘接体系中DOS、T27和GFP的迁移。结果表明,HTPB衬层和EPDM绝热层对DOS和T27的吸收能力很强;粘合剂的极性增大或交联密度升高,衬层对DOS、T27的吸收能力下降,但粘合剂的极性增大,对衬层与HTPB推进剂的界面粘接性能不利;在HTPB推进剂/HTPB衬层/EPDM绝热层粘接体系中,DOS、T27或GFP的迁移平衡浓度为粘合剂相的平衡浓度。 相似文献
990.
Sazonov V. V. Chebukov S. Yu. Abrashkin V. I. Kazakova A. E. Zaitsev A. S. 《Cosmic Research》2004,42(2):178-193
We analyze the microacceleration measurements carried out onboard the Foton-11 satellite with the three-component accelerometer BETA. The microaccelerations were recorded virtually throughout the entire orbital flight of the Foton-11 satellite. The data obtained were analyzed in the following way. First they were used to determine the actual rotational motion of the satellite for several arbitrarily selected time intervals 4 h long. This problem was solved by constructing the approximation of the microacceleretation low-frequency component (previously determined from the data) by its calculated analog computed along the solutions to differential equations of rotational motion of the satellite. The approximation was made by the least squares method. As a result, those mathematical model parameters and the solutions to equations of motion were found that gave the best consistency of the microacceleretation low-frequency component and its calculated analog. Then the spectral analysis of the low-frequency component and its calculated analog was made. It was shown that, although basic harmonics of these functions coincided sufficiently well, some harmonics of the low-frequency component failed to be interpreted in terms of the satellite's rotational motion. 相似文献