共查询到20条相似文献,搜索用时 156 毫秒
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1 前言自从对 IMP 和 OGO 卫星系统和部件进行磁试验以来,退磁已经做为一种把试验物体恢复到近零的原始磁状态的方法。1962年和1963年间,在部件磁试验设备(CMTF)中使用了直流退磁。近此时候完成的退磁试验是用60Hz 交流磁场退磁,代替了直流退磁。在一般的情况下,用初始磁场强度等于材料的矫顽力的磁场强度为铁磁材料退磁,肯定会退掉由材料磁性饱和引起的剩磁。 相似文献
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卫星整星充、退磁机理研究 总被引:1,自引:2,他引:1
文章从理论上阐述了卫星整星充、退磁的机理,对其中地磁场环境中退磁与零磁场环境中退磁的差别,地磁场环境中退磁的时效性,退磁频率、波形、幅值以及周期与退磁效果的关系,磁波形与退磁效果的关系,不同材料、不同尺度的情况下退磁的效果,充磁试验与地磁场环境中材料的充磁的差别以及卫星整星充、退磁试验中退磁场的选取等问题进行了详细的理论分析,对于卫星整星充、退磁试验技术有指导作用. 相似文献
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地磁场中卫星磁测试环境与设备 总被引:1,自引:0,他引:1
文章介绍了在地磁场中建立满足低轨道卫星运行的磁测试环境(低造价的低磁厂房)以及符合标准的磁测试仪器与设备的研制过程,对磁性的测量与控制进行了阐述。 相似文献
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对于磁洁净度要求严格的卫星在研制前要进行磁设计,研制过程中要进行磁控制,才能保证卫星磁性指标的实现.文章介绍了"探测一号"电磁验证模型星的磁设计与控制技术. 相似文献
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A new mathematical model of the uncontrolled rotational motion of the Foton satellite is presented. The model is based on the Euler dynamic equations of rigid body motion and takes into account the
action upon the satellite of four external mechanical moments: gravitational, restoring aerodynamic, moment with constant
components in the satellite-fixed coordinate system, and moment arising due to interaction of the Earth’s magnetic field with
the satellite’s proper magnetic moment. To calculate the aerodynamic moment a special geometrical model of the outer satellite
shell is used. Detailed form of the formulas giving above-mentioned moments in the equations of satellite motion is agreed
with the form of the considered motion. Model testing is performed by determining with its help the rotational motion of the
Foton M-2 satellite (it was in orbit from May 31, 2005 to June 16, 2005) using the data of the onboard measurements of the Earth’s
magnetic field strength. The use of the new model has led to a relatively small improvement in the accuracy of the motion
determination, but allowed us to obtain physically real estimates of some parameters. 相似文献
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Riazantseva M. O. Dalin P. A. Zastenker G. N. Parhomov V. A. Eselevich V. G. Eselevich M. V. Richardson J. 《Cosmic Research》2003,41(4):371-381
The results of a detailed study of large (by 20% and more) and sharp (faster than ten minutes) changes of the ion flux in the solar wind are presented. The data are provided by regular measurements onboard the INTERBALL-1 satellite in the period 1996–1999. Using statistical analysis, we obtained the distribution of these changes in their absolute and relative strength. It is shown that, for a considerable proportion of the events, such sharp and large changes of the ion flux (density) take place under conditions of fairly constant values of the solar wind velocity and of both the magnitude and components of the interplanetary magnetic field. 相似文献
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卫星综合电子系统现状和发展建议 总被引:4,自引:0,他引:4
文章首先总结了国内外卫星综合电子系统现状和发展趋势,在充分分析我国航天器对综合电子系统的需求的基础上,提出了我国卫星综合电子系统的发展思路。 相似文献
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Boguslavskii A. A. Sazonov V. V. Sokolov S. M. Zemskov V. S. Raukhman M. R. Shalimov V. P. 《Cosmic Research》2004,42(2):148-154
The periodicity of the structure of impurity heterogeneities in the longitudinal section of an indium antimonide monocrystal doped by tellurium (InSb:Te) is investigated. The monocrystal was grown by the method of floating zone melting onboard the Foton-3 satellite. It is shown that the frequencies of harmonic components of heterogeneities converted into the time region coincide with frequencies of microaccelerations in the range 0–0.005 Hz arising onboard the Foton satellites. This fact confirms the hypothesis stated previously that residual microaccelerations onboard the satellite were the cause of occurrence of indicated periodicities. 相似文献
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某航天小卫星的真空热试验 总被引:3,自引:3,他引:0
文章简要介绍了某航天小卫星真空热试验中对于试验工况的确定和外热流模拟方法的选择,通过试验验证了卫星热设计的正确,同时也指出外热流加热周期应与星内设备电测周期同步,必须充分考虑加热回路的承载能力,并注意试验设备导线漏热的影响,以及防止高温下挥发物质可能对光学组件的污染。 相似文献
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基于最小系统的小卫星在轨软件重构系统设计 总被引:3,自引:2,他引:1
提出一种基于星载终端处理设备最小系统的小卫星在轨软件重构系统设计方案。依据星上信息流实现现状,设计重构系统的系统框架,提出星载终端处理设备的最小系统组成、通用功能集和需要满足的整星安全性功能需求。系统中,应用软件程序数据按照注入帧格式通过遥控通道注入到星上,可缓存在星务存储器中再分发给终端目的设备,通过最小系统软件对应用程序进行引导和加载管理,整个过程均有差错控制设计以保证其可靠性和安全性。软件重构试验和容错试验表明,利用该系统可实现星载微计算机软件和FPGA配置数据的可靠上注、可靠存储和可靠加载。 相似文献
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The instrumental and applied problems related to the design of a passive magnetic attitude control system for the Munin nanosatellite are considered. The system is constructed from a strong permanent magnet and a set of hysteresis rods. These rods are made of magnetically soft material using a special technology, and they allow us to support the satellite orientation with respect to the local magnetic field vector with a given accuracy and time response. By using asymptotic and numerical methods, we investigate the satellite dynamics for different models of hysteresis. The issues concerning the arrangement of the rods and their interaction with the fields of permanent magnets mounted onboard the satellite are discussed. 相似文献