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101.
102.
N. Zolotukhina N. Polekh V. Kurkin O. Pirog S. Samsonov A. Moiseyev 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
We present an observational study of magnetospheric and ionospheric disturbances during the December 2006 intense magnetic storm associated with the 4В/Х3.4 class solar flare. To perform the study we utilize the ground data from North–East Asian ionospheric and magnetic observatories (60–72°N, 88–152°E) and in situ measurements from LANL, GOES, Geotail and ACE satellites. The comparative analysis of ionospheric, magnetospheric and heliospheric disturbances shows that the interaction of the magnetosphere with heavily compressed solar wind and interplanetary magnetic field caused the initial phase of the magnetic storm. It was accompanied by the intense sporadic E and F2 layers and the total black-out in the nocturnal subauroral ionosphere. During the storm main phase, LANL-97A, LANL 1994_084, LANL 1989-046 and GOES_11 satellites registered a compression of the dayside magnetosphere up to their orbits. In the morning–noon sector the compression was accompanied by an absence of reflections from ionosphere over subauroral ionospheric station Zhigansk (66.8°N, 123.3°E), and a drastic decrease in the F2 layer critical frequency (foF2) up to 54% of the quite one over subauroral Yakutsk station (62°N, 129.7°E). At the end of the main phase, these stations registered a sharp foF2 increase in the afternoon sector. At Yakutsk the peak foF2 was 1.9 time higher than the undisturbed one. The mentioned ionospheric disturbances occurred simultaneously with changes in the temperature, density and temperature anisotropy of particles at geosynchronous orbit, registered by the LANL-97A satellite nearby the meridian of ionospheric and magnetic measurements. The whole complex of disturbances may be caused by radial displacement of the main magnetospheric domains (magnetopause, cusp/cleft, plasma sheet) with respect to the observation points, caused by changes in the solar wind dynamic pressure, the field of magnetospheric convection, and rotation of the Earth. 相似文献
103.
Iliana Ilieva Tania Ivanova Yordan Naydenov Ivan Dandolov Detelin Stefanov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
Light is necessary for photosynthesis and shoot orientation in the space plant growth facilities. Light modules (LM) must provide sufficient photosynthetic photon flux for optimal efficiency of photosynthetic processes and also meet the constraints for power, volume and mass. A new LM for Svet space greenhouse using Cree® XLamp® 7090 XR light-emitting diodes (LEDs) was developed. Monochromic LEDs emitting in the red, green, and blue regions of the spectrum were used. The LED-LM contains 36 LED spots – 30 LED spots with one red, green and blue LED and 6 LED spots with three red LEDs. Digital Multiplex Control Unit controls the LED spots and can set 231 levels of light intensity thus achieving Photosynthetic Photon Flux Density (PPFD) in the range 0–400 μmol m−2 s−1 and different percentages of the red, green and blue light, depending on the experimental objectives. Two one-month experiments with plants – lettuce and radicchio were carried out at 400 μmol m−2 s−1 PPFD (high light – HL) and 220 μmol m−2 s−1 PPFD (low light – LL) and 70% red, 20% green and 10% blue light composition. To evaluate the efficiency of photosynthesis, in vivo modulated chlorophyll fluorescence was measured by Pulse Amplitude Modulation (PAM) fluorometer on leaf discs and the following parameters: effective quantum yield of Photosystem II (ΦPSII) and non-photochemical quenching (NPQ) were calculated. Both lettuce and radicchio plants grown at LL express higher photochemical activity of Photosystem II (PSII) than HL grown plants, evaluated by ΦPSII. Accelerated rise in NPQ in both LL grown plants was observed, while steady state NPQ values were higher in LL grown lettuce plants and did not differ in LL and HL grown radicchio plants. The extent of photoinhibition process in both plants was evaluated by changes in malonedialdehyde (MDA) concentration, peroxidase (POX) activity and hydrogen peroxide (H2O2) content. Accumulation of high levels of MDA and increased POX activity correlating with decreased H2O2 content were observed in both HL grown plants. These biochemical indicators revealed higher sensitivity to photodamage in HL grown lettuce and radicchio plants. LL conditions resulted in more effective functioning of PSII than HL when lettuce and radicchio plants were grown at 70% red, 20% green and 10% blue light composition. 相似文献
104.
无需先验信息的水平集SAR图像分割方法 总被引:1,自引:0,他引:1
给出了一种基于水平集演化、无需任何先验信息的SAR图像分割方法.该方法是一种基于区域信息的统计活动轮廓模型方法,通过利用分段阶跃函数估计图像概率密度函数,克服了利用特定概率分布模型估计概率密度函数时,需要利用先验信息预先假定图像概率分布模型的问题;通过引入惩罚项,避免了费时且难于操作的水平集函数重新初始化过程.还给出了具体的数值实现方案和相关参数取值,改进了数值实现中的迭代终止条件.实验结果表明,固定使用列出的参数,无需任何人为干预,对于大多数图像都可获得令人满意的分割结果;对于少数图像,通过简单的参数调整也可得到良好结果. 相似文献
105.
采用FLS900型稳态荧光光谱仪对激光持续照射的离体血液进行了荧光检测,得到了血液成分变化及荧光光谱特征随时间衰变的规律。实验结果表明:随着血液离体时间的延长,当受407nm的光激励时,605nm处的荧光峰峰位保持不变仅强度缓慢减弱。但在离体后的14h出现了谱形突变,并在474nm处产生了一个强荧光峰。分析认为,激光对离体血液的衰变有明显的延缓作用,但当激光持续照射一定时间后却导致了细胞的形态改变进而加速了细胞的溶血进程,产生了大量的内源性荧光物质还原烟碱腺嘌呤二核苷酸。研究结果为研究血细胞的活性衰变及细胞功能结构异常等提供了参考。 相似文献
106.
针对航天嵌入式系统中存在多级中断情况下的时间分析问题,提出了中断与任务混合的响应时间计算模型。该模型中断与任务使用统一的优先级定义,将多级中断嵌套的响应时间分析与任务嵌套的响应时间分析相结合,推导出了混合模型下响应时间计算公式。并进一步比较了中断与任务的异同,阐述了公式中关键参数的含义与计算方法。最后利用开源的LEON3平台和Modelsim软件对所述方法进行了仿真验证,结果表明,任务最差响应时间过估小于5%,可以得到准确的分析结果,有较高的工程应用价值。 相似文献
107.
108.
简述了自动拉平系统基本工作原理,对拉平轨迹及指数拉平规律进行分析,之后设计了自动拉平耦合器和拉平着陆系统。在MATLAB平台下,建立了自动拉平着陆系统结构图,并进行了大量仿真研究。仿真结果表明,所设计的自动拉平耦合器和拉平着陆系统参数合适、结构合理,系统工作稳定,并能满足预定的着陆参数要求。 相似文献
109.
M.A. Sharifi E. Forootan M. Nikkhoo J.L. Awange M. Najafi-Alamdari 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
The Caspian Sea has displayed considerable fluctuations in its water level during the past century. Knowledge of such fluctuation is vital for understanding the local hydrological cycles, climate of the region, and construction activities within the sea and along its shorelines. This study established a point-wise satellite altimetry approach to monitor the fluctuations of the Caspian Sea using a complete dataset of TOPEX/Poseidon for the period 1993 to the middle of 2002, and its follow-on Jason-1 for the period 2002 to August 2009. Therefore, 280 virtual time-series were constructed to monitor the fluctuations. The least squares spectral analysis (LSSA) method is, then employed to find the most significant frequencies of the time-series, while the statistical method of principle component analysis (PCA) is applied to extract the dominant variability of level variations. The study also used the observations of TOPEX/Poseidon and Jason-1 over the Volga River along with 5 years of Volga’s water discharge to study its influence on the Caspian Sea level changes. The LSSA results indicate that the lunar semidiurnal (M2) and the Sun semidiurnal (S2) frequencies are the main tidal frequencies of the Caspian Sea with the mean amplitude of 4.2 and 2.8 cm, respectively. A statistically significant long-term frequency (12.5-years period) is also found from altimetry and tide gauge observations. A phase lag, related to the inter-annual frequencies of the Volga River was detected from the point-wise time-series showing level propagation from the northwest to the southeast of the sea. The cross-correlation between the power spectrum of Volga and that of the northern-most, middle, and southern-most points within the Caspian Sea were respectively 0.63, 0.51 and 0.4 of zero-lag correlation, corroborating the influence of the Volga River. The result of PCA also shows that different parts of the Caspian Sea exhibit different amplitudes of level variations, indicating that the point-wise approach, when employing all available satellite measurements could be a suitable method for a preliminary monitoring of this inland water resource as it gives accurate local fluctuations. 相似文献
110.
旋转盘应力水平与温度分布的关联分析 总被引:1,自引:0,他引:1
基于有限元的热-弹性耦合算法,在等冷气耗量条件下,对旋转轮盘内应力水平与其表面温度分布的关联性进行了数值研究.在转速为 000 r/min,内、外缘温度分别为00℃和50℃条件下,盘面温度沿半径方向采用不同的"V"形变化时,得到了盘内等效应力水平随盘面温度分布变化的规律.计算结果表明:采用"V"形变化的盘面温度分布可以有效地降低盘内应力水平,说明了盘内应力水平与盘表面的温度分布存在着较强的关联性,在保证航空发动机整体气动性能的前提下,通过控制涡轮盘表面温度分布来有效降低轮盘的应力水平是可行的. 相似文献