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1.
内装式空射运载火箭重力出舱机箭耦合动力学分析 总被引:1,自引:1,他引:0
研究了以运输机为平台的内装式运载火箭空射过程载机和火箭的耦合动力学建模。建模针对两个阶段:第一阶段,火箭固定于载机机舱内,两者构成一个整体,按照普通刚体的力学方法处理;第二阶段,火箭解锁后,沿着舱内的发射筒向外滑行,载机和火箭形成两刚体相互作用的耦合系统,基于牛顿-欧拉法建立系统动力学模型。载机在空射火箭过程中,油门和升降舵满偏,在加速前飞的同时拉大姿态俯仰角,火箭在自身重力分量和惯性力的作用下,沿着机舱内的发射筒加速向外滑行,直至与载机分离。数值仿真分析了空射过程载机的重要力学参数的变化过程,验证了载机操控策略的可行性和安全性,可为未来中国空射运载火箭技术设计提供数据参考。 相似文献
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针对复杂动态环境下无人飞行器的动态障碍规避问题,基于合理假设建立了无人飞行器和动态障碍的运动学模型,并综合考虑无人飞行器飞行过程中的终端约束、控制输入约束、安全避障约束等,以能量最少为性能指标构建动态避障问题数学描述。之后,针对终端约束和控制输入约束,依据优化模型预测静态规划算法(OMPSP)生成初始轨迹;针对动态避障问题的不等式约束,引入松弛变量并结合滑模变结构控制方法设计松弛变量动力学,实现对一个、多个或同时多个动态障碍的安全规避;最后,依据有限时间微分动态规划(RHDDP)算法进行轨迹优化,获得满足上述各种约束并能规避动态障碍的近似最优轨迹。 相似文献
3.
随着我国航天事业的蓬勃发展,运载火箭发射要求也呈现多样化。北斗卫星导航系统是我国自行研制的全球卫星导航系统,经历三步跨越式发展,目前已经全面建成。CZ-3A系列火箭承担了北斗工程全部发射任务,该工程对火箭倾斜同步转移轨道(IGTO)、中圆转移轨道(MTO)、地球同步转移轨道(GTO)新类型轨道要求。介绍了该类轨道特点,讨论了火箭发射方案、发射轨道设计及高空风双向补偿方法。实际飞行考核充分证明了发射轨道设计的正确性,设计方法确保了北斗工程全部发射任务取得圆满成功,为北斗工程顺利实施奠定了基础。 相似文献
4.
《中国航空学报》2020,33(12):3206-3219
Topology optimization is an effective method to obtain a lightweight structure that meets the requirements of structural strength. Whether the optimization results meet the actual needs mainly depends on the accuracy of the material properties and the boundary conditions, especially for a tiny Flapping-wing Micro Aerial Vehicle (FMAV) transmission system manufactured by 3D printing. In this paper, experimental and numerical computation efforts were undertaken to gain a reliable topology optimization method for the bottom of the transmission system. First, the constitutive behavior of the ultraviolet (UV) curable resin used in fabrication was evaluated. Second, a numerical computation model describing further verified via experiments. Topology optimization modeling considering nonlinear factors, e.g. contact, friction and collision, was presented, and the optimization results were verified by both dynamic simulation and experiments. Finally, detailed discussions on different load cases and constraints were presented to clarify their effect on the optimization. Our methods and results presented in this paper may shed light on the lightweight design of a FMAV. 相似文献
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类IXV飞行器初期再入制导与姿态控制方法研究 《空间控制技术与应用》2018,44(3):22
摘要: 针对类IXV飞行器无翼式升力体构型及采用RCS/尾襟翼组合控制特点,研究其初期再入段的高精度制导与姿态控制方法.设计带过程约束的数值预测 校正制导律以提高制导系统的鲁棒性及精确性;根据其执行机构配置特点,设计基于RCS的航向控制律及基于RCS/气动舵的纵、横向复合控制律,并采用鲁棒伺服LQR技术进行控制参数快速设计.通过蒙特卡洛打靶仿真来验证算法的精度及鲁棒性. 相似文献
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本文讨论了舰载飞机以小于有利速度着舰时的航迹稳定性问题。在分析飞机航迹稳定性的同时,还对油门杆控制、机动襟翼控制对改善航迹稳定性的作用进行了初步探讨;在此基础上还讨论了舰载飞机加装波束导引系统对着舰过程的影响原理。结果表明:采用油门杆控制、机动襟翼控制来改善着舰阶段的航迹稳定性是可行的:而且用以上两控制系统作为内环的自动驾驶仪在波束导引系统自动导引飞机着舰过程中,能控制飞机的飞行速度、高度,帮助驾驶员操纵。 相似文献
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Emergence of a Habitable Planet 总被引:2,自引:0,他引:2
Kevin Zahnle Nick Arndt Charles Cockell Alex Halliday Euan Nisbet Franck Selsis Norman H. Sleep 《Space Science Reviews》2007,129(1-3):35-78
We address the first several hundred million years of Earth’s history. The Moon-forming impact left Earth enveloped in a hot
silicate atmosphere that cooled and condensed over ∼1,000 yrs. As it cooled the Earth degassed its volatiles into the atmosphere.
It took another ∼2 Myrs for the magma ocean to freeze at the surface. The cooling rate was determined by atmospheric thermal
blanketing. Tidal heating by the new Moon was a major energy source to the magma ocean. After the mantle solidified geothermal
heat became climatologically insignificant, which allowed the steam atmosphere to condense, and left behind a ∼100 bar, ∼500 K
CO2 atmosphere. Thereafter cooling was governed by how quickly CO2 was removed from the atmosphere. If subduction were efficient this could have taken as little as 10 million years. In this
case the faint young Sun suggests that a lifeless Earth should have been cold and its oceans white with ice. But if carbonate
subduction were inefficient the CO2 would have mostly stayed in the atmosphere, which would have kept the surface near ∼500 K for many tens of millions of years.
Hydrous minerals are harder to subduct than carbonates and there is a good chance that the Hadean mantle was dry. Hadean heat
flow was locally high enough to ensure that any ice cover would have been thin (<5 m) in places. Moreover hundreds or thousands
of asteroid impacts would have been big enough to melt the ice triggering brief impact summers. We suggest that plate tectonics
as it works now was inadequate to handle typical Hadean heat flows of 0.2–0.5 W/m2. In its place we hypothesize a convecting mantle capped by a ∼100 km deep basaltic mush that was relatively permeable to
heat flow. Recycling and distillation of hydrous basalts produced granitic rocks very early, which is consistent with preserved
>4 Ga detrital zircons. If carbonates in oceanic crust subducted as quickly as they formed, Earth could have been habitable
as early as 10–20 Myrs after the Moon-forming impact. 相似文献