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71.
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
72.
Nat Gopalswamy 《Space Science Reviews》2006,124(1-4):145-168
Interplanetary coronal mass ejections (ICMEs) originating from closed field regions on the Sun are the most energetic phenomenon
in the heliosphere. They cause intense geomagnetic storms and drive fast mode shocks that accelerate charged particles. ICMEs
are the interplanetary manifestations of CMEs typically remote-sensed by coronagraphs. This paper summarizes the observational
properties of ICMEs with reference to the ordinary solar wind and the progenitor CMEs. 相似文献
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75.
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
76.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(7):1685-1700
Pc4 signatures for the year 2013, extracted from geomagnetic north–south and east–west components of induction coil magnetometer (LEMI 30) from low latitude station Desalpar (DSP), operated by Institute of Seismological Research (ISR), India have been investigated vis-à-vis the prevalent interplanetary parameters (IMF) as well as the geomagnetic activity indices. A clear dominance of Pc4-5 (467 events) over Pc3 (17 events) is observed. Local time variation of Pc4 shows a peak in the noon sector in both X and Y components. Our investigations show that the dominant peak frequency is 10 mHz at low latitude region. Correlations with solar wind and IMF parameters illustrate highest occurrence of Pc4 for a solar wind speed of 300–400 km/s and average IMF B field of 3–6 nT. The amplitude of Pc4s at DSP shows an increase with increasing solar wind speed, plasma density, solar wind dynamic pressure and average B field which is also reflected in the trend of frequency variation of these pulsations. We report that IMF clock angle at low latitude does not have influence on Pc4 occurrence. Based on the characteristics of these events, detected in latitudinally distributed stations from low and mid-latitudes from northern and southern hemisphere, we infer that modes were compressional, which could be driven by K-H instability or solar wind dynamic pressure, as compressional modes can propagate to low latitude with little attenuation. 相似文献
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78.
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
79.
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
80.
在分析空空导弹战斗使用过程中影响导弹型号选择主要因素的基础上,提出了优选导弹型号的原则,并建立了数学模型;模拟结果表明,该原则充分反映了导弹的特性,因而是有效的。 相似文献