基于Transformer层次预测的多星应急观测任务规划方法

应急观测任务规划是一个强时效性的复杂组合优化问题,必须在规定的时限内完成相应的计算。采用机器学习的方法对规划问题进行初始规划方案预测,可以有效地简化计算复杂度。为此,提出一种基于Transformer层次预测的多星应急观测任务规划方法,将多星任务规划的求解过程分解为3个步骤：首先,利用基于Transformer的任务可调度性预测模型预测待规划任务是否执行,得到预执行任务集合;然后,基于Transformer的任务分配模型对预执行任务集合分配卫星,得到初始规划方案;最后,利用基于随机爬山的约束修正算法对初始规划方案进行优化调整,得到可行规划方案。为验证所提方法的有效性,通过大量仿真实验与CPLEX优化器、标准遗传算法、长短期记忆网络等方法模型进行比较,实验结果表明所提方法计算耗时短,规划收益高,适用于多星观测任务快速规划。     

过载环境下水平管内水的流动沸腾特性

利用地面离心旋转台实验研究了不同过载环境下水在1.8 mm内径水平管内流动沸腾的摩擦压降特性.实验工况为过载加速度1.00g～3.16g,质量流速为230、330 kg/(m2.s),热流密度为102、141 kW/m2,干度为0.07～0.58.结果表明:不同过载环境、干度、热流密度和质量流速对水的摩擦压降均有影响....     

对低轨导航系统发展趋势的思考CSCD

全球卫星导航系统成熟的产业推广和技术应用极大地牵引了卫星导航发展需求,使相关学者愈来愈关注恶劣电磁环境下的抗干扰技术以及分米、厘米级高精度导航定位服务。低轨星座优越的平台/轨道特性使其被誉为未来极具潜力的卫星导航手段。特别是近十年商业航天的蓬勃发展,带动卫星平台技术及火箭运载技术突飞猛进,大大降低了低轨卫星制造与发射成本,使得面向低轨星座的导航定位技术成为研究热点和发展方向。首先深入地剖析了不同历史阶段低轨导航的应用方向和技术体制,梳理归纳了低轨卫星星座独立定位及低中高轨卫星联合定位两种应用模式的技术特点,然后分析了未来低轨导航在整个卫星导航系统体系中的应用前景和技术挑战,为未来低轨导航系统建设和发展提供设计参考与技术借鉴。     

一种基于参数控制的低轨星载接收机载波跟踪算法CSCD

低轨星座接收机面临大多普勒频移及频繁快速换星等设计约束,对其载波跟踪环路设计提出了较高的动态适应性与跟踪精度要求。针对以上问题,提出了一种基于参数控制的载波跟踪算法。该算法引入环路控制因子参数,将环路滤波器分为牵引和跟踪两阶段。基于理论建模推导环路控制因子的最优参数配置原则,指导实现牵引和跟踪两种状态滤波器的协同配合,在牵引阶段有效引导大多普勒信号快速入锁,在跟踪阶段精确估计载波频移参数,实现基于低轨星载平台的GNSS信号快速准确跟踪。理论与仿真结果均表明基于参数控制的载波跟踪算法能够有效提升环路的动态适应性与跟踪精度,满足低轨星载接收机的设计需求。与传统算法相比,该算法在保证信号跟踪精度的同时,能够将收敛时间缩短78%,且环路设计简单,易于硬件实现。     

基于机器学习的单孔绝热气膜冷却效率分布预测研究

为了研究利用机器学习技术对绝热冷却效率进行直接预测的方法及特点,搭建了基于上采样卷积神经网络的机器学习模型,生成了用于训练以及验证的数值模拟数据集,使用了监督式学习的方法对模型进行了训练.训练使用反向传播算法和基于随机梯度下降的Adam优化算法,输入模型的参数包括吹风比、主流湍流强度、喷射角、孔形状、孔尺寸,模型输出为...     

Zonal mean temperature, pressure, zonal wind and geopotential height as functions of latitude

The new zonal mean COSPAR International Reference Atmosphere (CIRA-86) of temperature, zonal wind, and geopotential/geometric height is presented. This data can be used as a function of altitude or pressure and has nearly pole-to-pole coverage (80°S-80°N) extending from the ground to approximately 120 km. Data sources and methods of computation are described; in general, hydrostatic and thermal wind balance are maintained at all levels and latitudes. As shown by a series of cross sectional plots, the new CIRA accurately reproduces most of the characteristic features of the atmosphere such as the equatorial wind and the general structure of the tropopause, stratopause, and mesopause.     

Intrinsic time scale for reconnection on the dayside magnetopause

Recently much attention has been focused on the transient behavior of the magnetopause in response to pressure pulses and southward fluctuations of the interplanetary magnetic field. We examine the motion of the magnetopause behind the foreshock and conclude that this motion is affected by foreshock pressure variations but not by fluctuations in the direction of the magnetic field. Neither magnetopause erosion nor flux transfer event occurrence is controlled by the foreshock. On the contrary, flux transfer events occur at times of steady IMF and thier quasi-periodic behavior is controlled by the magnetopause or the magnetosphere and is not driven by the external boundary conditions. Since flux transfer events are clearly due to reconnection, this observation implies that the IMF must be southward some time perhaps as long as 7 minutes before flux transfer begins.     

Balloon altitude studies of southern hemisphere hard X-ray sources by the Imperial College-University of Tasmania-INPE collaboration

Hard X-ray balloon altitude measurements with a 1600 cm² phoswich array are described. Data from observations on Sco X-1, GX1+4, GX5−1, Nova Oph. 1977, SMC X-1, SS433, IC 4329A and MR 2251-178 are presented. The role of Comptonisation in X-ray production for Sco X-1 and GX1+4 is discussed.     

The 2.5 to 5 microns spectrum of comet Halley from the IKS instrument of Vega

Results of the 2.5–5 micron spectroscopic channel of the IKS instrument on Vega are reported and the data reduction process is described. H₂O and CO₂ molecules have been detected with production rates of 10³⁰ s⁻¹ and 1.5 10²⁸ s⁻¹ respectively. Emission features between 3.3 and 3.7 microns are tentatively attributed to CH - bearing compounds - CO is marginally detected with a mixing ratio CO/H₂O 0.2. OH emission and H₂O - ice absorption might also be present in the spectra.     

SIGMA observations of hard X-ray and soft gamma-ray emission from X-ray binaries

After more than two years of operation, the imaging γ-ray SIGMA telescope has accumulated several days of observation toward well known X-ray binaries. Four bright sources falling in this category have been detected so far: The pulsar GX 1+4 near the center of our galaxy, the stellar wind accreting system 4U 1700-377, and the black hole candidates Cygnus X-1 and GX 339-4. Moreover, SIGMA have observed three transients sources, which turned out to be also hard X-ray sources : The burster KS 1731-260, Tra X-1, and the Musca Nova. The properties of these systems in the SIGMA domain will be reviewed and a spectral distinction between black holes and neutron stars will be sketched.