排序方式: 共有27条查询结果,搜索用时 0 毫秒
21.
22.
一种适用于多波和半波点焊的恒流控制方法 总被引:2,自引:0,他引:2
影响点焊电流恒定输出的主要因素是网压波动和二次回路阻抗的变化,二次回路阻抗变化会导致负载功率类数角变化。理论分析表明:焊接电流有效值反映了网压波动和负载功率因数角的变化情况,对二者进行补偿,可实现恒流控制。本文所设计的恒流控制系统采用了恒热量输出的控制方式,利用焊接前检测网压有效值的方法,对网压波动和负载功率因数进行补偿,不断调整可控硅触发角,以保证恒流输出。实验结果表明:该控制系统既克服了因焊接电流来不及参与反馈控制调节而不能保证半波点焊恒流输出的缺陷,同时也适用于多不波点焊的恒流控制。 相似文献
23.
本文通过分析影响液浮挠性摆式加表K<,1>温度系数的各种因素,从加表的工作原理、结构特点、工艺过程等方面展开研究,系统介绍了加表K<,1>温度系数热磁补偿的理论计算和实验方法,大大提高了加表K<,1>温度系数合格率及K<,1>项精度. 相似文献
24.
通过介绍作者在工作中使用多项式拟合进行接收机频响补偿并取得的良好效果,说明多项式拟合是一种非常有用的工具。 相似文献
25.
在工程实施中双探头梯度法的误差系数只能达到0.5~0.3,意味着只能消除50%~70%的卫星剩磁干扰。文章研究双探头梯度法消除卫星本体剩磁的原理和工程上双探头梯度法的误差来源,并分析了卫星剩磁部件的分布对磁心的影响,以及磁心与双探头位置的关系在双探头梯度法中的关键作用。当磁心位置确定,并且双探头安装连线通过磁心,双探头梯度法的处理误差能够实现最小化。仿真试验表明,在优化剩磁部件分布和双探头部署位置的情况下,双探头梯度法的误差系数可以从0.4降低到0.03以下。 相似文献
26.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2023,71(4):2017-2037
Solar flares and coronal mass ejections (CMEs) cause immediate and adverse effects on the interplanetary space and geospace. In an era of space-based technical civilization, the deeper understanding of the mechanisms that produce them and the construction of efficient prediction schemes are of paramount importance. The source regions of flares and CMEs exhibit some common morphological characteristics, such as -spots, filaments and sigmoids, which are associated with strongly sheared magnetic polarity inversion lines, indicative of the complex magnetic configurations that store huge amounts of free magnetic energy and helicity. The challenge is to transform this empirical knowledge into parameters/predictors that can help us distinguish efficiently between quiet, flare-, and CME-productive (eruptive) active regions. This paper reviews these efforts to parameterize the characteristics of eruptive active regions as well as the importance of transforming new knowledge into more efficient predictors and including new types of data. Magnetic properties of active regions were first introduced when systematic ground-based observations of the photospheric magnetic field became possible and the relevant research was boosted by the provision of near real time, uninterrupted, high-quality observations from space, which allowed the study of large, statistically significant samples. Nonetheless, flare and CME prediction still faces a number of challenges. The magnetic field information is still constrained at the photospheric level and accessed only from one vantage point of observation, thus there is always need for better predictors; the dynamic behavior of active regions is still not fully incorporated into predictions; the inherent stochasticity of flares and CMEs renders their prediction probabilistic, thus benchmark sets are necessary to optimize and validate predictions. To meet these challenges, researchers have put forward new magnetic properties, which describe different aspects of magnetic energy storage mechanisms in active regions and offer the opportunity of parametric studies for over an entire solar cycle. This inventory of features/predictors is now expanded to include information from flow fields, transition region and coronal spectroscopy, data-driven modeling of the coronal magnetic field, as well as parameterizations of dynamic effects from time series. Further work towards these directions may help alleviate the current limitations in observing the magnetic field of higher atmospheric layers. In this task, fundamental and operational research converge, with promising results which could stimulate the development of new missions and lay the ground for future exploratory studies, also profiting from and utilizing the long anticipated observations of the new generation of instruments. 相似文献
27.