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对航天器太阳电池阵分流技术进行了归纳总结,对PWM,S3R和S4R三种开关分流调节技术进行了详细的原理分析,比较总结各自的技术特点。并对S3R和S4R技术进行了深入研究,对S3R技术进行了详细的设计与计算,对S4R技术典型工况进行了详细分析与实验验证。同时对三种开关分流技术做出了评价。 相似文献
606.
为了研究Halo轨道中继通信以及行星际轨道转移等问题,需要首先对拉格朗日点(平动点)的理论进行分析。使用考虑太阳辐射的椭圆型限制性三体建模,代替原有的圆型限制性三体建模,提高了建模的精度。提出了在L1,L2,L3点的更为精确的新解析解,经过Matlab仿真,其相对于精确数值解的误差,分别为Ammar的解析解的13.13%,29.51%,0.46%。 相似文献
607.
G.A. Bazilevskaya 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
Many physical processes precede and accompany the solar energetic particles (SEP) occurrence on the Earth’s orbit. Explosive energy release on the Sun gives rise to a flare and a coronal mass ejection (CME). X-ray and gamma emissions are believed to be connected with flares. Radio emission is signature of disturbances traveling through the corona and interplanetary space. Particles can gain energy both in the flare and the accompanying wave processes. The beginning of the SEP events has the advantage of being the phase most close to the time of acceleration. Influence of interplanetary transport is minimal in the case of first arriving relativistic solar protons recorded by ground based neutron monitors in so called ground-level enhancements (GLE). The early phase of the SEP events attracts attention of many scientists searching for the understanding of particle acceleration. However, they come to the opposite conclusions. While some authors find arguments for coronal mass ejections as a sole accelerator of SEPs, others prove a flare to be the SEP origin. Here, the circumstances of SEP generation for several GLEs of the 23rd solar cycle are considered. Timing of X-ray, CME, and radio emissions shows a great variety from event to event. However, the time of particle ejection from the Sun is closer to maximum of X-ray emission than to any other phenomena considered. No correlation is found between the particle fluxes and the CME characteristics. 相似文献
608.
牵顶伞在降落伞拉直过程中的作用 总被引:1,自引:0,他引:1
采用有限元方法,建立降落伞回收系统的多质点动力学模型,研究了牵顶伞在拉直过程中对主伞性能的影响.模型中将柔性大变形的伞绳、伞表、连接带离散成若干绳段,各绳段假设为质量集中在中心的质点,各质点间以阻尼弹簧连接,其运动由对应绳段的重力、气动力和张力确定.利用该模型对某批次的空投试验进行了仿真,给出了张力、速度、位移等参数的瞬态变化.经过分析表明,牵顶伞能够改善主伞张力分布,抑制伞衣项部横向摆动. 相似文献
609.
Since November 1978 a complete set of total solar irradiance (TSI) measurements from space is available, yielding a time series of 21 years. From measurements made by different space radiometers (HF on NIMBUS-7, ACRIM I on SMM, ACRIM II on UARS and VIRGO on SOHO) a composite record of TSI can be compiled. The corrections which are needed for each radiometer, mainly to compensate for degradation, but also for operational influences are described. ACRIM I (1980–1989) and ACRIM II (1992–1995) are taken as reference because their degradation was monitored by inflight comparisons with spare radiometers; since 1996 VIRGO is used as reference. The scale of ACRIM II is adjusted to ACRIM I by comparison with NIMBUS-7 and ERBE. The reliability of this adjustment depends strongly on the stability of the HF and ERBE radiometer during the period of the gap between the ACRIMs which is discussed in detail together with an assessment of the overall precision of the composite. 相似文献
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