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231.
Solar proton events recorded in the stratosphere during cosmic ray balloon observations in 1957–2008
G.A. Bazilevskaya V.S. MakhmutovY.I. Stozhkov A.K. SvirzhevskayaN.S. Svirzhevsky 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
Long-term balloon observations have been performed by the Lebedev Physical Institute since 1957 up to the present time. The observations are taken several times a week at the polar and mid latitudes and allow us to study dynamics of galactic and solar cosmic ray as well as secondary particle fluxes in the atmosphere and in the near-Earth space. Solar energetic particles (120) – mostly protons – (SEP) events with >100 MeV proton intensity above 1 cm−2 s−1 s−1 were recorded during 1958–2006. Before the advent of the SEP monitoring on spacecraft these results constituted the only homogeneous series of >100 MeV SEP events. The SEP intensities and energy spectra inferred from the Lebedev Physical Institute observations are consistent with the results taken in the adjacent energy intervals by the spacecraft and neutron monitors. Joint consideration of the SEP events series recorded by balloons and by neutron monitors during solar cycles 20–23 makes it possible to restore the probable number of events in solar cycle 19, which was not properly covered by observations. Some correlation was found between duration of SEP event production in a solar cycle and sunspot cycle characteristics. 相似文献
232.
233.
“资源一号”卫星火工控制系统设计的正确性、合理性和可靠性、安全性,与卫星成败有着非常密切的联系。文章重点描述了“资源一号”卫星火工控制系统可靠性安全性的设计,主要包括火工控制系统的点火电路设计、点火通路电缆设计、太阳电池板(文中简称太阳翼)可靠展开的冗余设计和点火限流电阻的设计等4方面内容,尤其在点火限流电阻的选取和设计方面进行了完善和提高。 相似文献
234.
235.
太阳同步轨道卫星的太阳帆板驱动规律研究 总被引:1,自引:0,他引:1
翟坤 《空间控制技术与应用》2008,34(4):38-41
研究一类斜飞斜装特殊的太阳同步轨道卫星。首先确定太阳帆板的开始驱动时刻,并给出地球阴影区的计算方法,然后根据不同情况分析太阳帆板的过程驱动规律,并提出基于MATLAB/Simulink/RTW软件的数值设计方法,最后以某卫星为例,说明太阳帆板驱动规律的设计过程,并得到满足工程需要的结果,验证该设计方法的准确性和可行性。 相似文献
236.
A study on the resistance performance of epoxy nano-composites under the vacuum ultraviolet irradiation 总被引:2,自引:0,他引:2
Irradiation damage effects of the epoxy resin 648 and epoxy nano-composites are studied by means of simulating the vacuum ultraviolet (VUV) irradiation whose wavelength ranges from 5 to 200 nm. Experimental results of the mass loss, SEM and XPS show that nano-TiO2 particles exhibit better resistance performance under VUV. Comparing with epoxy resin, the epoxy nano-composite brings significantly less mass loss, slighter flexural strength variation and decreasing gas extraction with less gas component varieties after irradiation. What is more, no new carbon peak-value has been found and principle components of Ols peak-value remain unchanged on the surface. 相似文献
237.
238.
根据Ylysses观测,比较完整地计算了高纬行星际空间太阳风能流分布.计算表明,行星际空间的高速流能流密度约为2.1×10-3J·m-2·s-1(日心距离r=1AU),主要来自于太阳风离子所携带的动能流(占58%)和克服太阳引力的势能流(占39%).要驱动高速流,需要在日冕底部高速流源区(日心距离r=1Rs)向外输出到太阳风的能流密度为7.1×102J·m-2·s-1·分析表明,由日冕底部向外可能输出两种形式的能流,其中一种具有较短的耗散长度,被耗散在很短的空间区域(~1—2Rs),使日冕温度迅速提高。另一种储藏在连续向外传播的太阳风中,不断耗散用以加速太阳风(>2Rs). 相似文献
239.
Recent papers have suggested that the slow solar wind is a super-position of material which is released by reconnection from
large coronal loops. This reconnection process is driven by large-scale motions of solar magnetic flux driven by the non-radial
expansion of the solar wind from the differentially rotating photosphere into more rigidly rotating coronal holes.
The elemental composition of the slow solar wind material is observed to be fractionated and more variable than the fast solar
wind from coronal holes. Recently, it has also been reported that fractionation also occurs in 3He/4He. This may be interpreted
in the frame-work of an existing model for fractionation on large coronal loops in which wave-particle interactions preferentially
heat ions thereby modifying their scale-heights.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
240.
立方星在轨任务期间的能源供给主要依靠蓄电池或体装太阳能电池阵。随着微小航天器技术的发展,立方星功能密度越来越大,星上载荷对功率的需求越来越高,传统的电池板供能方式已很难满足未来空间任务需求。另外,立方星因其特有的尺寸规范和标准,对电池阵的收纳尺寸和展开机构也有特殊应用需求。基于上述背景和立方星的结构特点,设计了一种展开原理简单、扩展性好、折展比大的一维剪叉式空间可展开机构,进行了原理样机的加工制造和地面展开试验,验证了机构设计的功能可行性以及设计参数的合理性。机构展开后阵列发电功率是传统供能方式的3~5倍,且特殊的几何外形可提供被动重力梯度稳定优势,在提升未来立方星载荷能力方面有重要应用价值。 相似文献