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101.
Balázs Pintér R. Erdélyi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(2):759-776
Solar fundamental (f) acoustic mode oscillations are investigated analytically in a magnetohydrodynamic (MHD) model. The model consists of three layers in planar geometry, representing the solar interior, the magnetic atmosphere, and a transitional layer sandwiched between them. Since we focus on the fundamental mode here, we assume the plasma is incompressible. A horizontal, canopy-like, magnetic field is introduced to the atmosphere, in which degenerated slow MHD waves can exist. The global (f-mode) oscillations can couple to local atmospheric Alfvén waves, resulting, e.g., in a frequency shift of the oscillations. The dispersion relation of the global oscillation mode is derived, and is solved analytically for the thin-transitional layer approximation and for the weak-field approximation. Analytical formulae are also provided for the frequency shifts due to the presence of a thin transitional layer and a weak atmospheric magnetic field. The analytical results generally indicate that, compared to the fundamental value (), the mode frequency is reduced by the presence of an atmosphere by a few per cent. A thin transitional layer reduces the eigen-frequencies further by about an additional hundred microhertz. Finally, a weak atmospheric magnetic field can slightly, by a few percent, increase the frequency of the eigen-mode. Stronger magnetic fields, however, can increase the f-mode frequency by even up to ten per cent, which cannot be seen in observed data. The presence of a magnetic atmosphere in the three-layer model also introduces non-permitted propagation windows in the frequency spectrum; here, f-mode oscillations cannot exist with certain values of the harmonic degree. The eigen-frequencies can be sensitive to the background physical parameters, such as an atmospheric density scale-height or the rate of the plasma density drop at the photosphere. Such information, if ever observed with high-resolution instrumentation and inverted, could help to gain further insight into solar magnetic structures by means of solar magneto-seismology, and could provide further insight into the role of magnetism in solar oscillations. 相似文献
102.
微藻航空燃料的热氧化安定性与热沉 总被引:1,自引:0,他引:1
航空燃料安定性和热沉对飞机和发动机工作可靠性、飞机飞行安全及战术性能的发挥有重要作用。利用热重-差热分析联用仪研究了2种典型微藻航油的热氧化安定性和热沉,并与标准航空喷气燃料RP-3进行了对比。结果表明:混合生物油的失重终点温度和最大失重点的温度与标准航空喷气燃料RP-3相比均向高温区移动。在失重区间内,除了物理热沉还有化学热沉的贡献。在热重曲线中定义了2个无量纲参数:引发温度和燃尽指数,引发温度表征起始裂解温度,燃尽指数表征沉积特性。2个参数结合可以较好地诠释燃料的热安定性和热沉。球等鞭金藻油高碳数烷烃在提高热沉基础上导致碳沉积的形成,但小球藻油在热沉提高的基础上,并没有形成碳沉积。说明通过有效控制高碳数烷烃分配比例增加其热沉并控制其积碳在理论和技术上是可行的。 相似文献
103.
104.
辐射带高能电子通量波动与地磁暴警报 总被引:1,自引:1,他引:0
地球磁场捕获带电粒子形成辐射带,地磁场的扰动将导致带电粒子通量的变化.根据磁暴期间外辐射带高能电子通量起伏和波动的特点及规律,利用GOES卫星实时发布的5min分辨率高能电子微分通量数据,构建了高能电子通量波动指数,并分析了该指数与地磁活动的关系.结果表明,所提出的高能电子通量波动指数与地磁事件有很好的相关性,能起到地磁暴发生的指示剂作用,相对于目前空间环境业务化预报过程中广泛使用的3hKp指数,高能电子通量波动指数能更早地警报地磁暴的发生,是潜在有效的地磁暴警报辅助手段,能为空间环境预报中的地磁暴实时警报提供重要参考. 相似文献
105.
水下图像成像过程中,每个场景点所对应的光线在传播过程中均经过多种折射率不同的介质,因此水下图像会产生折射变形,导致传统基于单视点相机模型的水下图像三维重构方法精度极大降低.在理论分析一个新的单视点调节模型对水下图像折射变形的补偿能力的基础上,提出一种高效、自动的水下图像三维重构及其非线性优化方法.为了验证该方法的性能,利用合成数据和真实图像对其进行测试,并依据重构有效性、重构误差等定量指标考察分析了实验结果.实验结果表明,提出的多视图水下三维重构方法可有效补偿水下场景成像空间变形,进而显著提高传统基于单视点相机模型的水下三维重构质量. 相似文献
106.
样本重复使用失效响应曲线分析结构可靠度方法 总被引:1,自引:0,他引:1
用基于样本重复使用失效响应曲线逼近法,为充分利用迭代过程中的样本点,提出了样本重复使用的思想,并由此发展出一种结构可靠度的计算方法.利用可靠度指标作为收敛条件,从迭代收敛后的所有样本点中选取靠近失效界线处的样本点构造失效曲线响应函数,最后通过蒙特卡洛抽样的方法计算可靠度.多个算例表明:该响应函数避免了对传统意义上的功能函数响应面的模拟,降低了模型维数,又由于适当地 引入了带交叉项、具有曲线旋转功能的响应函数,因此能够很好地逼近失效曲线,有效地提高可靠度计算精度. 相似文献
107.
Using 86 CME-interplanetary shock events,the correlation between the peak values of (a) the solar wind parameters(Bz,Ey,Pdyn) and the geomagnetic indices(SYM-H,ASY-H,Kp), (b) the coupling functions(Borovsky,Akasofu,Newell) and the geomagnetic indices,(c) the solar wind parameters/coupling functions/geomagnetic indices and the ionospheric parameter(Δf0F2min), are investigated.The statistical results show that in group(a),Bz min and SYM-Hmin have the best correlation,that in group(b),the best correlation is between the peak values of Akasofu function (Amin) and SYM-Hmin,and that in group(c),the best correlation is between Kpmax andΔf0F2min. Based on the statistical results,a method for predicting f0F2 of a single station is attempted to be set up.The input is modified Bz min and the outputs are SYM-Hmin andΔf0F2min.Then 25 CME-IPS events that caused geomagnetic storms in 1998 and 2009 are used to check the prediction method. The results show that our method can be used to predict SYM-Hmin andΔf0F2min. 相似文献
108.
S. Shimada J. Matsumoto A. Sekiyama B. Aosier M. Yokohana 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
The objectives of the present study were to develop a new index based on remotely-sensed data for detecting the abundance of grasses in the family Poaceae, which has a high palatability for livestock in Mongolia, and to map the distribution of these grasses in the semi-arid Mongolian steppes. We measured ground-based spectral reflectance of pure plant leaves – including Poaceae grasses – and soils, as well as in-situ in the Mongolian grasslands. The hyper-spectral data, taken by a spectroradiometer, were converted into four multi-spectral bands (i.e., blue, green, red, and NIR) to simulate satellite-based imagery data. In order to magnify the characteristics of the spectral signal of Poaceae, NGBDI (Normalized Green-Blue Difference Index), NGRDI (Normalized Green-Red Difference Index), NDVI (Normalized Difference Vegetation Index), NNBDI (Normalized NIR-Blue Difference Index) were calculated from the four multi-spectral reflectance values. Poaceae Abundance Index (PAI) was derived by combining these four normalized difference indices. PAI was found out to be a good indicator to discriminate Poaceae grass from the other plant spectral data. 相似文献
109.
Soybean cultivar selection for Bioregenerative Life Support Systems (BLSSs) – Hydroponic cultivation
R. Paradiso R. Buonomo V. De Micco G. Aronne M. Palermo G. Barbieri S. De Pascale 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
Four soybean cultivars (‘Atlantic’, ‘Cresir’, ‘Pr91m10’ and ‘Regir’), selected through a theoretical procedure as suitable for cultivation in BLSS, were evaluated in terms of growth and production. Germination percentage and Mean Germination Time (MGT) were measured. Plants were cultivated in a growth chamber equipped with a recirculating hydroponic system (Nutrient Film Technique). Cultivation was performed under controlled environmental conditions (12 h photoperiod, light intensity 350 μmol m−2 s−1, temperature regime 26/20 °C light/dark, relative humidity 65–75%). Fertigation was performed with a standard Hoagland solution, modified for soybean specific requirements, and EC and pH were kept at 2.0 dS m−1 and 5.5 respectively. 相似文献
110.
综述了国内外开展飞行器健康相关研究的现状,强调了考虑渐变过程对于健康仿真的重要性。以某型飞行器电动舵机为研究对象,建立了舵机系统的非线性仿真模型。通过分析组成电动舵机各个环节的健康模式与模型参数的映射关系,阐述了建立健康模型开展健康仿真的方法,并结合测点仿真数据和多维向量相似度、遗传算法的原理,提出了健康指标的计算和优化方法,达到健康评估的目的。最后,以simulink环境下的仿真实例对上述方法的可行性进行了初步验证。 相似文献