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81.
82.
扇翼飞行器的研究进展与应用前景 总被引:4,自引:0,他引:4
随着科学技术的迅猛发展,飞机无论在构型还是性能方面都获得了飞速发展,但是新原理飞机的研制却进展不大。扇翼飞行器是近期发展起来的低速大载荷新型飞行器,它是不同于现有固定翼、旋翼飞行器的新构型、新原理飞行器。而国内对于该飞行器的研究才刚刚起步,可参考的文献资料很少。因此,本文通过国内外扇翼飞行器发展状况的研究,对扇翼飞行器研究进展进行总结分析。首先介绍了扇翼飞行器的飞行原理;其次系统地回顾了扇翼飞行器的提出,并总结了其在国内外研究的进展情况;接着根据扇翼飞行器近期的发展动态,对该飞行器的应用前景作出分析;最后总结了扇翼飞行器发展中亟待解决的关键技术,以及其未来发展的难点和趋势。 相似文献
83.
Introduction
The current U.S. extravehicular activity (EVA) suit in space includes liquid cooling and ventilation garment (LCVG) to control thermal condition. Tubes knitted in LCVG for flowing water interrupt evaporation of perspiration, and astronauts feel discomfort. In the present study, we hypothesized that a self-perspiration garment would effectively lower the skin temperature without raising humidity in the garment. Thus, we developed and examined the effects of the garment.Methods
Eight healthy subjects were studied with a cyclic ergometer of 30, 60 90 and 120 W loading for 3 min each. Skin temperature and humidity on the back were measured continuously. Subjects wore and tested three types of garments i.e., a spandex wear without any cooling device (Normal), a simulated LCVG (s-LCVG) or the spandex wear knitted a vinyl tube for flowing water, and the spandex wear with a tube, which flows water and self-perspiration with oozing water for evaporative cooling (SPEC).Results
All measurements were reached to steady state 2–3 min after the setting. The s-LCVG decreased skin temperature 0.39±0.14 °C during 12 min of cooling. With SPEC, skin temperature did not decrease significantly until 6–9 min after starting the cooling. However, the temperature decreased rapidly and significantly after that, and finally decreased 1.59±0.32 °C. Humidity in the SPEC was significantly lower than that in s-LCVG.Discussion
SPEC was effective for lowering skin temperature without raising humidity in the garment. The concept is expected to use as a better cooling system during EVA. 相似文献84.
跟踪研究了美国海基激光武器的发展动态,论述了其发展历程、基本构成、作战流程和发展现状,剖析了其关键技术的攻关进展情况,预测了其未来作战应用,并得出相应结论。 相似文献
85.
Fridrich Valach Josef Bochníček Pavel Hejda Miloš Revallo 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The paper deals with the relation of the southern orientation of the north–south component Bz of the interplanetary magnetic field to geomagnetic activity (GA) and subsequently a method is suggested of using the found facts to forecast potentially dangerous high GA. We have found that on a day with very high GA hourly averages of Bz with a negative sign occur at least 16 times in typical cases. Since it is very difficult to estimate the orientation of Bz in the immediate vicinity of the Earth one day or even a few days in advance, we have suggested using a neural-network model, which assumes the worse of the possibilities to forecast the danger of high GA – the dominant southern orientation of the interplanetary magnetic field. The input quantities of the proposed model were information about X-ray flares, type II and IV radio bursts as well as information about coronal mass ejections (CME). In comparing the GA forecasts with observations, we obtain values of the Hanssen–Kuiper skill score ranging from 0.463 to 0.727, which are usual values for similar forecasts of space weather. The proposed model provides forecasts of potentially dangerous high geomagnetic activity should the interplanetary CME (ICME), the originator of geomagnetic storms, hit the Earth under the most unfavorable configuration of cosmic magnetic fields. We cannot know in advance whether the unfavorable configuration is going to occur or not; we just know that it will occur with the probability of 31%. 相似文献
86.
M. Pietrella M. PezzopaneC. Bianchi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
Hourly systematic measurements of the highest frequency reflected by the sporadic-E layer (foEs) recorded from January 1976 to June 2009 at the ionospheric stations of Rome (Italy, 41.8°N, 12.5°E) and Gibilmanna (Italy, 37.9°N, 14.0°E) were considered to carry out a comparative study between the sporadic E layer (Es) over Rome and Gibilmanna. Different statistical analysis were performed taking into account foEs observations near the periods of minimum and maximum solar activity. The results reveal that: (1) independently from the solar activity, Es develops concurrently over extended regions in space, instead of being a spatially limited layer which is transported horizontally by neutral winds over a larger area; especially during summer months, when an Es layer is present at Rome, there is a high probability that an Es layer is also present over Gibilmanna, and vice versa; (2) Es layer lifetimes of 1–5 h were found; in particular, Es layers with lifetimes of 5 h both over Gibilmanna and Rome are observed with highest percentages of occurrence in summer ranging between 80% and 90%, independently from the solar activity; (3) latitudinal effects on Es layer occurrence emerge mostly for low solar activity during winter, equinoctial, and summer months, when Es layers are detected more frequently over Gibilmanna rather than Rome; (4) when the presence of an Es layer over Rome and Gibilmanna is not simultaneous, Es layer appearance both over Rome and Gibilmanna confirms to be a locally confined event, because drifting phenomena from Rome to Gibilmanna or vice versa have not been emphasized. 相似文献
87.
为解决研制阶段装备群保障规模预测的问题,建立了基于保障活动流程的装备群保障规模预测模型.模型从装备群的使用任务入手,以研制阶段保障性分析和保障系统建模数据为输入,通过分析资源在保障活动中被占用或被消耗的定量关系,从占用型资源和消耗型资源两方面分别提供了由功能分析框图中各层保障活动的流程汇总保障活动资源需求的方法,对保障资源数量进行计算,进而依据这些资源的重量与体积参数预测装备群的保障规模.给出了某型机群保障规模预测的算例,验证了模型的合理性与工程适用性,能够为研制阶段装备保障的改进、系统部署性分析提供理论指导与技术支持. 相似文献
88.
Periodic Variations of Drag Coefficient for the ANDE Spherical Satellites During its Lifetime
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A drag coefficient (CD) inversion method is introduced to study the variations of the drag coefficient for orbital satellites with spherical geometry. Drag coefficients of the four micro satellites in the Atmospheric Neutral Density Experiment (ANDE) are compiled out with this new method. The Lomb-Scargle Periodgram (LSP) analysis of the four ANDE satellites' CD series has shown that there are obvious 5, 7, 9, and 27 days' period in those data. Interesting results are found through comparing the LSP analysis with series of the daily solar radio flux at 10.7 cm (F10.7 index), the Ap index, and the daily averaged solar wind speed at 1AU. All series in the same time interval have an obvious period of about 27 days, which has already been explained as the association with the 27 days' solar rotation. The oscillating periods less than 27 days are found in series of CD, Ap and solar wind speed at 1AU, e.g., the 5, 7, 9 days period. However, these short periods disappeared in the time series of F10.7 index. The same periodicities of 5, 7, 9 days in Ap and solar wind are presented at the same time interval during the declining phase of solar cycle 23. While in the ascending phase of solar cycle 24, these short oscillations are not so obvious as that in the declining phase of solar cycle 23. These results provide definite evidence that the CD variations with period of 5, 7 and 9 days are produced by a combination of space weather effects caused by the solar wind and geomagnetic activity. 相似文献
89.
维修性设计是军用飞机保障特性设计重要工作之一,随着数字化设计手段的广泛应用,为适应军用飞机数字化设计平台环境,满足维修性设计评价的型号工作需求,本文以数字化产品系统为基础,构建了包括产品数字化设计、维修任务仿真、维修性分析评价为一体的维修性评价平台。针对某型飞机光电探测设备整体组件拆装情况,依据构建的维修性评价数字化平台实际工作流程,本文最后介绍了在飞机设计阶段,如何开展对光电探测设备整体组件拆装的维修性验证评价。 相似文献
90.
S.V. Veretenenko V.A. DergachevP.B. Dmitriyev 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
Long-term changes of the Arctic frontal zone characteristics near the south-eastern coasts of Greenland were considered, the NCEP/NCAR reanalysis data being used. It was found that in the cold half of the year the temperature gradients in the layer 1000–500 hPa in the region under study reveal strong ∼10-yr and ∼22-yr periodicities that seem to be related to solar activity cycles. The results obtained suggest the influence of solar activity and cosmic ray variations on the structure of the temperature field of the troposphere resulting in the changes of the temperature contrasts in the Arctic frontal zone that, in turn, may affect the intensity of cyclogenesis at middle latitudes. The detected effects seem to indicate an important part of frontal zones in the mechanism of solar activity and cosmic ray variation influence on the development of extratropical baric systems. It is suggested that the variations of the temperature gradients revealed in the Arctic frontal zone are due to the radiative forcing of cloudiness changes which may be associated with geomagnetic activity and cosmic ray variations. 相似文献