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111.
112.
Kh. Karami S. Ghader A. Raeen 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
In the present work values of peak electron density (NmF2) and height of F2 ionospheric layer (hmF2) over Tehran region at a low solar activity period are compared with the predictions of the International Reference Ionosphere models (IRI-2001 and IRI-2007). Data measured by a digital ionosonde at the ionospheric station of the Institute of Geophysics, University of Tehran from July 2006 to June 2007 are used to perform the calculations. Formulations proposed by and are utilized to calculate the hmF2. The International Union of Radio Science (URSI) and International Radio Consultative Committee (CCIR) options are employed to run the IRI-2001 and IRI-2007 models. Results show that both IRI-2007 and IRI-2001 can successfully predict the NmF2 and hmF2 over Tehran region. In addition, the study shows that predictions of IRI-2007 model with CCIR coefficient has closer values to the observations. Furthermore, it is found that the monthly average of the percentage deviation between the IRI models predictions and the values of hmF2 and NmF2 parameters are less than 10% and 21%, respectively. 相似文献
113.
O.S. Oyekola 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
We use hourly monthly median values of propagation factor M(3000)F2 data observed at Ouagadougou Ionospheric Observatory (geographic12.4°N, 1.5°W; 5.9o dip), Burkina Faso (West Africa) during the years Januar1987–December1988 (average F10.7 < 130 × 10−22 W/m2/Hz, representative of low solar flux conditions) and for January 1989–December1990 (average F10.7 ? 130 × 10−22 W/m2/Hz, representative of high solar epoch) for magnetically quiet conditions to describe local time, seasonal and solar cycle variations of equatorial ionospheric propagation factor M(3000)F2 in the African region. We show that that seasonal trend between solar maximum and solar minimum curves display simple patterns for all seasons and exhibits reasonable disparity with root mean square error (RMSE) of about 0.31, 0.29 and 0.26 for December solstice, June solstice and equinox, respectively. Variability Σ defined by the percentage ratio of the absolute standard deviation to the mean indicates significant dissimilarity for the two solar flux levels. Solar maximum day (10–14 LT) and night (22–02 LT) values show considerable variations than the solar minimum day and night values. We compare our observations with those of the IRI 2007 to validate the prediction capacity of the empirical model. We find that the IRI model tends to underestimate and overestimate the observed values of M(3000)F2, in particular, during June solstice season. There are large discrepancies, mainly during high solar flux equinox and December solstice between dawn and local midnight. On the other hand, IRI provides a slightly better predictions for M(3000)F2 between 0900 and 1500 LT during equinox low and high solar activity and equinox high sunspot number. Our data are of great importance in the area of short-wave telecommunication and ionospheric modeling. 相似文献
114.
本文提出一种重量信号的无线传输和测量方法。重量信号经传感顺转换成电信号,再经V/F变换后调频发射,接收信号解调后单片机处理。单片机的信号处理采用电子计数器测频方法,经过计算送显示单元,实现重量信号的遥测。 相似文献
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黄春峰 《航空精密制造技术》2004,40(3):16-19
主要叙述了H13、QRO80M、QRO90SUPREME等新型热作模具钢的性能、使用特点及其热处理工艺技术方法。 相似文献
117.
Zhigang Yuan Baiqi Ning Xiaohua Deng 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009,44(9):1013-1018
Based on observations of two ionosondes at Wuhan and Kokubunji, this paper presents effects of TADs on the daytime mid-latitude ionosphere during the intense geomagnetic storm on March 31, 2001. During a positive ionospheric storm, the start of the enhancement of the foF2 (F2 peak plasma frequency) at Wuhan lags that at Kokubunji by 15 min, which corresponds to the time interval of traveling atmospheric disturbances (TADs’) propagation from Kokubunji to Wuhan. Associated with the uplifting of the hmF2 (height of F2 peak) caused by TADs, it is observed by the two ionosondes that the F1 cusp becomes better developed. Therefore, during a geomagnetic storm, TADs originating from the auroral oval may have a strong influence on the shape of the electron density profile in the F1 region ionosphere at middle latitudes. It is highly likely that TADs are responsible for the evolution of the F1 cusp. 相似文献
118.
一类空间对称6R机构的运动学研究及组合应用 总被引:1,自引:0,他引:1
可展开平板机构已广泛应用于平板天线、太阳翼等航天机构产品。为提高可展开平板机构的刚度和展收比,将空间对称6R机构应用于可展开平板机构设计。首先,根据约束条件,计算后给出了一种空间3R运动链的几何参数关系;然后,结合螺旋理论,分析了该3R运动链的约束螺旋系;进而根据对称性,研究了空间对称6R机构的自由度、奇异性等运动特征;在此基础上,提出了一种特殊的空间对称6R转动机构;最后,研究了空间对称6R机构的组合方法,设计出一种新型单自由度可展开平板组合机构,并对其进行了运动学仿真验证。该可展机构具有二维方向的展开收拢能力,为可展开平板机构的创新设计提供了有益参考。 相似文献
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针对变频技术的核心—SPWM波形的产生和控制,详细介绍了SPWM波形的产生方法,并给出了软件编程。通过以DSP芯片TMS320F2812为核心,利用规则采样法产生SPWM波形,具有速度快,精度高,实时控制能力强,易于频率变换等优点。 相似文献