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Kohei Fujimoto Daniel J. Scheeres Johannes Herzog Thomas Schildknecht 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The direct Bayesian admissible region approach is an a priori state free measurement association and initial orbit determination technique for optical tracks. In this paper, we test a hybrid approach that appends a least squares estimator to the direct Bayesian method on measurements taken at the Zimmerwald Observatory of the Astronomical Institute at the University of Bern. Over half of the association pairs agreed with conventional geometric track correlation and least squares techniques. The remaining pairs cast light on the fundamental limits of conducting tracklet association based solely on dynamical and geometrical information. 相似文献
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本文利用北京天文台提供的高空间分辨率的活动区纵场磁图对1988年的18个活动区进行分析研究,以寻求强SWF耀斑的先兆.结果表明,一磁流在异极性磁流区浮现,同极性磁流合并、异极性磁流侵入和纵向磁场强度剧增4种磁位形演化与强SWF耀斑有密切关系。文中还用1988年9—10月份的25个活动区的磁图和耀斑资料佐证上面的结果。 相似文献
54.
对SPOT遥感图象的信息保持型压缩编码进行了研究。对几种不同的预测器及A_2、A_3线性码进行了比较,得出如下结论:在SPOT 遥感图象的信息保持型压缩编码中,采用文献[1]提出的三点预测器较好,线性码采用A_3码较好;两者结合,在信息保持率大于99%时,可使压缩比达2倍以上。文内还对在压缩图象的传输与恢复中碰到的问题进行了探讨。 相似文献
55.
太阳电子事件粒子源区的位置 总被引:1,自引:0,他引:1
对ISEE-3的引个太阳电子事件资料,进行了系统地分析。通过Saha平衡模型分别计算了高Fe事件和贫Fe事件源区的平衡温度大小,指出两类事件粒子源区不相重合,高Fe事件的粒子源区位于高色球层,贫Fe事件粒子源区在色球层-日冕之间的过渡区。对高Fe事件和贫Fe事件的形成作了初步的设想。 相似文献
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Erika Gularte Daniel D. Carpintero Juliana Jaen 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(7):1790-1802
We have developed a new approach towards a new database of the ionospheric parameter . This parameter, being the frequency of the maximum of the ionospheric electronic density profile and its main modeller, is of great interest not only in atmospheric studies but also in the realm of radio propagation. The current databases, generated by CCIR (Committee Consultative for Ionospheric Radiowave propagation) and URSI (International Union of Radio Science), and used by the IRI (International Reference Ionosphere) model, are based on Fourier expansions and have been built in the 60s from the available ionosondes at that time. The main goal of this work is to upgrade the databases by using new available ionosonde data. To this end we used the IRI diurnal/spherical expansions to represent the variability, and computed its coefficients by means of a genetic algorithm (GA). In order to test the performance of the proposed methodology, we applied it to the South American region with data obtained by RAPEAS (Red Argentina para el Estudio de la Atmósfera Superior, i.e. Argentine Network for the Study of the Upper Atmosphere) during the years 1958–2009. The new GA coefficients provide a global better fit of the IRI model to the observed than the CCIR coefficients. Since the same formulae and the same number of coefficients were used, the overall integrity of IRI’s typical ionospheric feature representation was preserved. The best improvements with respect to CCIR are obtained at low solar activities, at large (in absolute value) modip latitudes, and at night-time. The new method is flexible in the sense that can be applied either globally or regionally. It is also very easy to recompute the coefficients when new data is available. The computation of a third set of coefficients corresponding to days of medium solar activity in order to avoid the interpolation between low and high activities is suggested. The same procedure as for can be perfomed to obtain the ionospheric parameter M(3000)F2. 相似文献
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航空发动机机匣摆线粗加工轨迹规划方法 总被引:1,自引:0,他引:1
针对机匣零件粗加工过程中凸台多、加工余量大、材料难切削、刀具磨损快、加工周期长等特点,提出了一种机匣摆线粗加工刀具轨迹规划方法,该方法能有效控制切削过程中刀具负载的变化,改善刀具切削过程中的加热-冷却循环,减缓刀具的磨损,提高机匣粗加工效率。首先,通过对两种摆线模型的分析,建立了摆线铣数学模型,并分析了摆线铣的优缺点;其次,结合机匣零件特点,将模型在精度范围内离散为点模型,利用圆锥将模型展开并建立展开模型与原始模型间的映射关系。通过对可加工区域的划分和平面逼近,生成了适用于机匣零件的摆线粗加工刀具轨迹。最后,分别通过摆线铣刀具磨损实验、平面型腔摆线铣实验和机匣摆线铣实验,验证了摆线铣在降低刀具磨损、延长刀具寿命方面的有效性,以及本文轨迹生成算法在航空发动机机匣实际加工中的正确性和高效性。研究成果能有效缩短加工周期、降低加工成本,提升机匣零件的粗加工效率。 相似文献
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60.
A.J. de Abreu P.R. Fagundes M. Gende O.S. Bolaji R. de Jesus C. Brunini 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The responses of the ionospheric F region using GPS–TEC measurements during two moderate geomagnetic storms at equatorial, low-, and mid-latitude regions over the South American and African sectors in May 2010, during the ascending phase of solar cycle 24, are investigated. The first moderate geomagnetic storm studied reached a minimum Dst value of −64 nT at 1500 UT on 02 May 2010 and the second moderate geomagnetic storm reached a minimum Dst value of −85 nT at 1400 UT on 29 May 2010. In this paper, we present vertical total electron content (VTEC) and phase fluctuations (in TECU/min) from Global Positioning System (GPS) observations from the equatorial to mid-latitude regions in the South American and African sectors. Our results obtained during these two moderate geomagnetic storms from both sectors show significant positive ionospheric storms during daytime hours at the equatorial, low-, and mid-latitude regions during the main and recovery phases of the storms. The thermospheric wind circulation change towards the equator is a strong indicator that suggests an important mechanism is responsible for these positive phases at these regions. A pre-storm event that was observed in the African sector from low- to the mid-latitude regions on 01 May 2010 was absent in the South American sector. This study also showed that there was no generation or suppression of ionospheric irregularities by storm events. Therefore, knowledge about the suppression and generation of ionospheric irregularities during moderate geomagnetic storms is still unclear. 相似文献