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101.
机型成本预测的因素分析法 总被引:1,自引:1,他引:0
根据管理会计把机型成本要素分解为固定成本、半变动成本和变动成本,对航空公司机型的航空运量作出预测,就可对机型作出预测。 相似文献
102.
103.
A.M. Unewisse 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(3):1026-1038
Mean night-time peak power, Doppler shift and Doppler width of spread Doppler clutter (SDC) received by a high frequency backscatter radar located at Alice Springs, Australia from 2000 to 2018 is presented as a function of azimuth, sunspot number, time of year and frequency. The sampled region covers 90 degrees from West to North and includes the northern and southern equatorial anomalies.SDC peak power diminished across all azimuths during the winter solstice from around May to August (local winter) coinciding with the global decrease in F layer density due to the annual non-seasonal F2 anomaly but was generally constant during the equinoxes. In contrast, SDC Doppler width and inbound Doppler shift both increased during the equinoxes and exhibited azimuthal dependence related to the eastward equatorial plasma drift.SDC peak power increased with increasing sunspot number with frequency dependence during winter but not summer. Inbound Doppler shift and Doppler width increased with increasing sunspot number during equinox but not solstice with a strong dependence on azimuth and a weak dependence on frequency. 相似文献
104.
Mohamed Nedal M. Youssef Ayman Mahrous Rabab Helal 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(5):1824-1836
We studied a set of 74 CMEs, with shedding the light on the halo-CMEs (HCMEs), that are associated with decametric – hectometric (DH) type-II radio bursts (1–16?MHz) and solar flares during the period 2008–2014. The events were classified into 3 groups (disk, intermediate, and limb events) based on their longitudinal distribution.We found that the events are mostly distributed around 15.32° and 15.97° at the northern and southern solar hemispheres, respectively. We found that there is a clear dependence between the longitude and the CME’s width, speed, acceleration, mass, and kinetic energy. For the CMEs’ widths, most of the events were HCMEs (~62%), while the partial HCMEs comprised ~35% and the rest of events were CMEs with widths less than 120°. For the CMEs’ speeds, masses, and kinetic energies, the mean values showed a direct proportionality with the longitude, in which the limb events had the highest speeds, the largest masses, and the highest kinetic energies. The mean peak flux of the solar flares for different longitudes was comparable, but the disk flares were more energetic. The intermediate flares were considered as gradual flares since they tended to last longer, while the limb flares were considered as impulsive flares since they tended to last shorter.A weak correlation (R?=?0.32) between the kinetic energy of the CMEs and the duration of the associated flares has been noticed, while there was a good correlation (R?=?0.76) between the kinetic energy of the CMEs and the peak flux of the associated flares. We found a fair correlation (R?=?0.58) between the kinetic energy of the CMEs and the duration of the associated DH type-II radio bursts. 相似文献
105.
106.
研究了1995年10月24日日食过程中,我国低纬地区广州和海口的F2层临界频率f0F2的高干扰重心频率ICF变化过程,鉴于多次日 处低纬的两地f0F2的日食变化形态不完全一样,以及多次日食期间同一地方f0F2变化形态不完全一样,ICF也并不像预想的那样降低,因而对于低纬电离层,动力学过程可能要比直接与太阳辐射有关的光化学过程起更为重要的作用。 相似文献
107.
根据微波网络理论提出了利用A参量求解高频阻抗的新方法,并将其应用于网络分析仪系统,对短波阻抗进行了测量。实践证明,该方法与传统的利用S参量的方法(利用反射系数)相比大大地拓宽了阻抗测量范围,在通用仪器上获得了比专用仪器高的测量精度,同时还解决了网络分析仪与非同轴网络的连接问题。 相似文献
108.
提供了一个计算副翼配重着陆冲击响应的方法。由于主起落架为纯摇臂式,考虑机体的弹性,机体和主起落架运动联立求解的加速度不是显式,因此必须用高斯方法解加速度的线性方程组,再用吉尔方法解微分方程。 相似文献
109.
用织女一号火箭在海南站探测的高空风和风切变 总被引:7,自引:4,他引:3
本文介绍了织女一号(ZN-l)火箭测风原理,数据处理方法和两次测风结果.结果指出,在我国低纬地区中层大气中存在非常明显的风切变和相当强的重力波扰动,测风数据与COSPAR国际参考大气CIRA1986及国际标准化组织航空用参考大气ISO5878-1982/ADD.1-1983存在明显差别. 相似文献
110.
片切磨削方法构造的自由曲面磨削支持系统 总被引:1,自引:0,他引:1
以操作者高效准确操作数控磨削中心为目的,开发了自由曲面磨削支持系统,进行了基于球头磨具的磨削中心基础研究。讨论了获得高精度曲面的加工要点,并提出了片切磨削方法。 相似文献