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31.
N. Wichaipanich P. Supnithi T. Tsugawa T. Maruyama T. Nagatsuma 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
In this work, the foF2 and hmF2 parameters at the conjugate points near the magnetic equator of Southeast Asia are studied and compared with the International Reference Ionosphere (IRI) model. Three ionosondes are installed nearly along the magnetic meridian of 100°E; one at the magnetic equator, namely Chumphon (10.72°N, 99.37°E, dip angle 3.0°N), and the other two at the magnetic conjugate points, namely Chiang Mai (18.76°N, 98.93°E, dip angle 12.7°N) and Kototabang (0.2°S, 100.30°E, dip angle 10.1°S). The monthly hourly medians of the foF2 and hmF2 parameters are calculated and compared with the predictions obtained from the IRI-2007 model from January 2004 to February 2007. Our results show that: the variations of foF2 and hmF2 predicted by the IRI-2007 model generally show the similar feature to the observed data. Both parameters generally show better agreement with the IRI predictions during daytime than during nighttime. For foF2, most of the results show that the IRI model overestimates the observed foF2 at the magnetic equator (Chumphon), underestimates at the northern crest (Chiang Mai) and is close to the measured ones at the southern crest of the EIA (Kototabang). For hmF2, the predicted hmF2 values are close to the hmF2(M3000F2OBS) during daytime. During nighttime, the IRI model gives the underestimation at the magnetic equator and the overestimation at both EIA crests. The results are important for the future improvements of the IRI model for foF2 and hmF2 over Southeast Asia region. 相似文献
32.
Daan Stevenson Hanspeter Schaub 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
The use of electrostatic (Coulomb) actuation for formation flying is attractive because non-renewable fuel reserves are not depleted and plume impingement issues are avoided. Prior analytical electrostatic force models used for Coulomb formations assume spherical spacecraft shapes, which include mutual capacitance and induced effects. However, this framework does not capture any orientation-dependent forces or torques on generic spacecraft geometries encountered during very close operations and docking scenarios. The Multi-Sphere Method (MSM) uses a collection of finite spheres to represent a complex shape and analytically approximate the Coulomb interaction with other charged bodies. Finite element analysis software is used as a truth model to determine the optimal sphere locations and radii. The model is robust to varying system parameters such as prescribed voltages and external shape size. Using the MSM, faster-than-realtime electrostatic simulation of six degree of freedom relative spacecraft motion is feasible, which is crucial for the development of robust relative position and orientation control algorithms in local space situational awareness applications. To demonstrate this ability, the rotation of a cylindrical craft in deep space is simulated, while charge control from a neighboring spacecraft is used to de-spin the object. Using a 1 m diameter craft separated by 10 m from a 3 by 1 m cylindrical craft in deep space, a 2 °/s initial rotation rate can be removed from the cylinder within 3 days, using electric potentials up to 30 kV. 相似文献
33.
S.P. Kuzin S.K. Tatevian S.G. Valeev V.A. Fashutdinova 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
An accuracy of geocenter motion estimation is strongly dependent on the geodetic network size and stations distribution over the Earth’s surface. From this point of view DORIS system has an advantage, as its ground network of beacons consists of more than 50 sites, equally distributed over the Earth’s surface. Aiming to study variations of the geocenter movements, the results of DORIS data analysis for the time span 1993.0–2009.0 (inawd06.snx series), performed at the Analysis Centre of the Institute of astronomy of the Russian Academy of Sciences, have been used. DORIS data processing was made with GIPSY/OASIS II software, developed by Jet Propulsion Laboratory and modified for DORIS data processing by Institute Géographique National. Standard deviations of stations coordinates are estimated at the level 0.5–4.0 cm (internal consistency), depending on the number of satellites used in the solution. RMS of estimated components of the DORIS satellites orbits, compared with the solutions of other IDS analysis centres, do not exceed 1–2 cm. Weekly solutions for coordinates have been transformed from free network solutions (inawd06.snx series) to a well defined terrestrial reference frame ITRF2005 with the use of seven parameters of Helmert transformation, which were examined with a view to study variations of the geocenter movements (ina05wd01.geoc time series). In order to estimate linear trend, amplitudes, periods and phases of geocenter variation a method of linear regression was applied. The evaluated amplitudes of annual variations are of the order of 5–7 mm for X and Y components and 27–29 mm for Z component. Semi-annual amplitudes are also noticeable in all components (1–34 mm for X, Y and Z components). Secular trends in the DORIS geocenter coordinates are: −1.2, −0.1 and −0.3 mm/year for X, Y and Z directions respectively. 相似文献
34.
N.V. Kuznetsov N.I. Nikolaeva 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
The proton fluxes from the low-Earth orbital satellites databases (NPOES-17 and CORONAS-F) were analyzed for the quiet geomagnetic period in April 2005. The satisfactory consent was found between the experimental and the AP8 model fluxes of the trapped protons with energy more than ∼10 MeV. At the same time, trapped proton fluxes with energy less than 10 MeV measured by LEO satellites were higher than the ones predicted by the AP8 model in the region of the SAA (drift shell L < 1.5). 相似文献
35.
Internet资源的指数级增长促进了个性化服务的发展.针对传统的用户兴趣建模方法在准确率和增量处理能力方面的不足,提出了一种新的基于概念聚类的用户兴趣建模方法UIM2C2(User Interest Modeling Method based on Conceptual Clustering).该方法首先通过分析用户访问的历史文档构造后缀树结构,然后选择不同的相似度阈值,以不同的粒度合并基本簇.依据不同阈值条件下合并的基本簇之间的包含关系,生成用户的兴趣层次.UIM2C2方法是针对文档的一个增量式、无监督的概念学习方法,因此用户描述文件可以轻易的获取和更新.最后,通过数据集20NewsGroup上的实验验证了UIM2C2方法在兴趣预测方面的有效性. 相似文献
36.
G. Boscheri M. Kacira L. Patterson G. Giacomelli P. Sadler R. Furfaro C. Lobascio M. Lamantea L. Grizzaffi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
Models are required to accurately predict mass and energy balances in a bioregenerative life support system. A modified energy cascade model was used to predict outputs of a multi-crop (tomatoes, potatoes, lettuce and strawberries) Lunar greenhouse prototype. The model performance was evaluated against measured data obtained from several system closure experiments. The model predictions corresponded well to those obtained from experimental measurements for the overall system closure test period (five months), especially for biomass produced (0.7% underestimated), water consumption (0.3% overestimated) and condensate production (0.5% overestimated). However, the model was less accurate when the results were compared with data obtained from a shorter experimental time period, with 31%, 48% and 51% error for biomass uptake, water consumption, and condensate production, respectively, which were obtained under more complex crop production patterns (e.g. tall tomato plants covering part of the lettuce production zones). These results, together with a model sensitivity analysis highlighted the necessity of periodic characterization of the environmental parameters (e.g. light levels, air leakage) in the Lunar greenhouse. 相似文献
37.
38.
Q. Wang G. Xu S. Petrovic U. Schaefer U. Meyer T. Xu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
A regional tropospheric model can be constructed using surveys from GPS ground networks. Using this model the tropospheric delays of a kinematic station within the region can be interpolated. However, such a model is generally not suitable for an airborne platform high above the ground networks. In this paper, a method of constructing a regional tropospheric model for airborne GPS applications is described. First, the kinematic station in the air is projected onto the ground. Then the tropospheric delays at projected point are interpolated from those of the ground networks. Finally, the tropospheric delays at projected point are extended upward to the airborne platform using pressure and temperature gradients and humidity exponential function. For validation of this method, the data of airborne campaign carried out by BKG in cooperation with GFZ and BGR 2008 in the northern Alps are used. The results show that GPS kinematic positioning precision in height component can be improved using this method. 相似文献
39.
为提高超磁致伸缩致动器(GMA)的设计效率,建立了GMA动力学模型和ANSYS有限元模型,对其轴向谐振频率进行了计算和模拟,并进行了GMA轴向谐振频率分析实验。通过实验数值和计算值及有限元分析结果的对比,动力学模型计算所得的GMA轴向谐振频率与实验值的误差小于5%, ANSYS分析所得的GMA轴向谐振频率与实验值的误差小于3%,验证了动力学模型和有限元模型的有效性。最后,通过ANSYS有限元分析了GMA各部件对其轴向谐振频率的影响,并提出利用有限元分析来提高GMA的结构刚度从而改善其轴向谐振频率的方法。 相似文献
40.
<正> 对某机种碳纤维复合材料垂尾加强肋、座舱盖、垂尾蒙皮等构件进行模态分析试验,所采用的试验方法如图1所示。 相似文献