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391.
杨丰 《长沙航空职业技术学院学报》2013,13(2):61-64
文章阐述了变螺距螺纹加工的编程方法,探讨了用宏程序实现变螺距螺纹的参数化编程,提高了编程效率,增强了程序的灵活性和通用性。 相似文献
392.
S.G. Wang J.K. Shi X. Wang G.J. Wang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
NeQuick ionospheric electron density model, which has been developed to version 2, produces the full electron density profile in the ionosphere. Each part of the profile is modeled using Epstein layer formalism. Simple empirical relations are used to compute the thicknesses of each layer. In order to validate the B2bot parameter in the NeQuick model during high solar activity, we use the data at Hainan, China (109.1°E, 19.5°N; Geomagnetic coordinates: 178.95°E, 8.1°N), measured with DPS-4, and study the diurnal and seasonal variations of B2bot, ΔB2 (B2best − B2NeQuick 2) and the seasonal median values of B2best/B2NeQuick 2 at that region. The results show that, (1) The differences between B2best and B2NeQuick 2 have diurnal and seasonal variations. (2) The diurnal variations of B2NeQuick 2 are smaller than those of B2best. (3) Generally, except for early morning the experimental values are properly reproduced. (4) Generally, during morning the NeQuick model has an underestimation. The magnitude of underestimation varies with LT and season. 相似文献
393.
Dipak Debnath Sandip K. Chakrabarti Anuj Nandi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
The Galactic black hole candidate H 1743-322 exhibited two X-ray outbursts in rapid succession: one in August 2010 and the other in April 2011. We analyze archival data of this object from the PCA instrument on board RXTE (2–25 keV energy band) to study the evolution of its temporal and spectral characteristics during both the outbursts, and hence to understand the behavioral change of the accretion flow dynamics associated with the evolution of the various X-ray features. We study the evolution of QPO frequencies during the rising and the declining phases of both the outbursts. We successfully fit the variation of QPO frequency using the Propagating Oscillatory Shock (POS) model in each of the outbursts and obtain the accretion flow parameters such as the instantaneous shock locations, the shock velocity and the shock strength. Based on the degree of importance of the thermal (disk black body) and the non-thermal (power-law) components of the spectral fit and properties of the QPO (if present), the entire profiles of the 2010 and 2011 outbursts are subdivided into four different spectral states: hard, hard-intermediate, soft-intermediate and soft. We attempt to explain the nature of the outburst profile (i.e., hardness-intensity diagram) with two different types of mass accretion flow. 相似文献
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396.
邱鹏瑞 《西安航空技术高等专科学校学报》2012,(1):67-68
目的搭建学校、企业、学生三方合作交流平台,加强高职院校顶岗实习过程管理与监控;方法根据学生顶岗实习需求,结合.net平台和数据库技术;结果设计实现基于B/S结构的顶岗实习网络管理系统;结论有助于确保顶岗实习质量,提高人才培养的水平。 相似文献
397.
杨晓新 《西安航空技术高等专科学校学报》2008,26(1):73-74
以创新型、综合型实验设计为目标,通过对流体力学综合实验台功能的设计与开发,突出其综合应用性和对实践教学效果的促进作用;对实验数据进行分析,说明实验台设计的合理性。 相似文献
398.
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S.M. Kopeikin E. Pavlis D. Pavlis V.A. Brumberg A. Escapa J. Getino A. Gusev J. Müller W.-T. Ni N. Petrova 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,42(8):1378-1390
Lunar laser ranging (LLR) measurements are crucial for advanced exploration of the laws of fundamental gravitational physics and geophysics as well as for future human and robotic missions to the Moon. The corner-cube reflectors (CCR) currently on the Moon require no power and still work perfectly since their installation during the project Apollo era. Current LLR technology allows us to measure distances to the Moon with a precision approaching 1 mm. As NASA pursues the vision of taking humans back to the Moon, new, more precise laser ranging applications will be demanded, including continuous tracking from more sites on Earth, placing new CCR arrays on the Moon, and possibly installing other devices such as transponders, etc. for multiple scientific and technical purposes. Since this effort involves humans in space, then in all situations the accuracy, fidelity, and robustness of the measurements, their adequate interpretation, and any products based on them, are of utmost importance. Successful achievement of this goal strongly demands further significant improvement of the theoretical model of the orbital and rotational dynamics of the Earth–Moon system. This model should inevitably be based on the theory of general relativity, fully incorporate the relevant geophysical processes, lunar librations, tides, and should rely upon the most recent standards and recommendations of the IAU for data analysis. This paper discusses methods and problems in developing such a mathematical model. The model will take into account all the classical and relativistic effects in the orbital and rotational motion of the Moon and Earth at the sub-centimeter level. The model is supposed to be implemented as a part of the computer code underlying NASA Goddard’s orbital analysis and geophysical parameter estimation package GEODYN and the ephemeris package PMOE 2003 of the Purple Mountain Observatory. The new model will allow us to navigate a spacecraft precisely to a location on the Moon. It will also greatly improve our understanding of the structure of the lunar interior and the nature of the physical interaction at the core–mantle interface layer. The new theory and upcoming millimeter LLR will give us the means to perform one of the most precise fundamental tests of general relativity in the solar system. 相似文献
400.