The History and Dynamics of Comet 9P/Tempel 1

Since its discovery in 1867, periodic comet 9P/Tempel 1 has been observed at 10 returns to perihelion, including all its returns since 1967. The observations for the seven apparitions beginning in 1967 have been fit with an orbit that includes only radial and transverse nongravitational accelerations that model the rocket-like thrusting introduced by the outgassing of the cometary nucleus. The successful nongravitational acceleration model did not assume any change in the comet’s ability to outgas from one apparition to the next and the outgassing was assumed to reach a maximum at perihelion. The success of this model over the 1967–2003 interval suggests that the comet’s spin axis is currently stable. Rough calculations suggest that the collision of the impactor released by the Deep Impact spacecraft will not provide a noticeable perturbation on the comet’s orbit nor will any new vent that is opened as a result of the impact provide a noticeable change in the comet’s nongravitational acceleration history. The observing geometries prior to, and during, the impact will allow extensive Earth based observations to complement the in situ observations from the impactor and flyby spacecraft.     

1978—1988年间磁扰的分析与日地耦合

用1978-1988年间行星际磁场(IMF)的B_z分量、极光区AL指数和赤道附近地磁台Z分量等资料探讨了日地耦合中的主要物理过程。B_z的11年变化大致与太阳活动程度相当,但AL和赤道附近ΔZ更多地受磁层和电离层内部过程所控制。分析中强调了对国际磁抗日按物理过程进行分类的必要性。      

风洞投放试验技术的研究现状与应用综述

多体分离是航空、航天和武器系统总体部门一直极为关注的关键问题,多体间的流场干扰效应产生的气动力和力矩对悬挂物分离相容性有重要影响,基于运动动力学相似的风洞投放试验技术是预测和评估多体分离是否相容的一种非定常试验方法。根据飞行器多体分离相容性的研究需求,结合作者在风洞投放试验技术的研究成果和经验,对风洞投放试验技术的国内外研究现状进行综述。首先回顾了风洞投放试验技术的发展历史,然后对低速和高速风洞投放试验的相似准则及缩比关系进行详细地论述与分析,进而对风洞投放试验的几个关键技术进行综述,最后对风洞投放试验技术存在的问题提出思考与展望。     

仪器舱惯组支架角振动传递特性分析

大型的仪器舱角振动试验对试验能力提出了新要求,仿真计算十分必要。建立了仪器舱和惯组小系统的有限元模型,研究了惯组系统置于仪器舱支架上后角振动传递特性的变化规律,分析了线角交联响应特性。分析表明,放置于支架上的惯组角振动传递特性变得恶劣,而且线振动输入下交联响应较大。研究结论对于仪器舱角振动试验的实施具有很大价值。     

行星齿轮系动力学特性分析及试验研究

采用集中质量法,考虑时变刚度、齿侧间隙、太阳轮的横向与纵向位移、太阳轮和行星轮的偏心误差激励,建立了行星齿轮传动系统的非线性动力学模型。采用龙塔库特法求解了系统的响应、相图、频谱图和动力学均载系数;通过测量系统齿根应力的动载荷应变图,获得齿根应变变形的相图、频谱图和系统的均载系数。研究结果表明:理论分析结果与试验测试结果比较吻合,说明采用的理论研究方法是合理的,测试方案是可行的。     

电磁屏蔽抗干扰技术研究

从干扰源性质出发,将屏蔽分为电场屏蔽、磁场屏蔽和电磁场屏蔽,并对它们进行了分析研究。针对其特性提出其适用范围及注意事项,从而增强了抗干扰的效果。     

New Insights on Geomagnetic Storms from Model Simulations Using Multi-Spacecraft Data

The forecast of the terrestrial ring current as a major contributor to the stormtime Dst index and a predictor of geomagnetic storms is of central interest to ‘space weather’ programs. We thus discuss the dynamical coupling of the solar wind to the Earth's magnetosphere during several geomagnetic storms using our ring current-atmosphere interactions model and coordinated space-borne data sets. Our model calculates the temporal and spatial evolution of H⁺, O⁺, and He⁺ ion distribution functions considering time-dependent inflow from the magnetotail, adiabatic drifts, and outflow from the dayside magnetopause. Losses due to charge exchange, Coulomb collisions, and scattering by EMIC waves are included as well. As initial and boundary conditions we use complementary data sets from spacecraft located at key regions in the inner magnetosphere, Polar and the geosynchronous LANL satellites. We present recent model simulations of the stormtime ring current energization due to the enhanced large-scale convection electric field, which show the transition from an asymmetric to a symmetric ring current during the storm and challenge the standard theories of (a) substorm-driven, and (b) symmetric ring current. Near minimum Dst there is a factor of ∼ 10 variation in the intensity of the dominant ring current ion specie with magnetic local time, its energy density reaching maximum in the premidnight to postmidnight region. We find that the O⁺ content of the ring current increases after interplanetary shocks and reaches largest values near Dst minimum; ∼ 60% of the total ring current energy was carried by O⁺ during the main phase of the 15 July 2000 storm. The effects of magnetospheric convection and losses due to collisions and wave-particle interactions on the global ring current energy balance are calculated during different storm phases and intercompared. This revised version was published online in August 2006 with corrections to the Cover Date.     

直升机旋翼黏弹阻尼器时域动力学建模与分析

建立一种适用于旋翼气动弹性分析的黏弹阻尼器模型,该模型考虑了黏弹材料本身的刚度非线性及激振力频率和幅值对黏弹阻尼器应力-应变关系的影响。通过引入新型几何非线性弹簧模块,根据需要调整模型的刚度变化规律,避免了现有黏弹阻尼器模型模拟不同类型材料时因刚度变化规律差异而需重新建模的缺陷,模型适应性强。模型采用多个内变量场,既能体现阻尼器幅变特性,也能准确反映多频激励下的黏弹性特性。以两种不同类型黏弹材料制造的黏弹阻尼器为研究对象,在旋翼黏弹阻尼器的典型工作幅值和频率范围内,进行了简谐实验。利用建立的旋翼黏弹阻尼器非线性时域动力学模型,计算不同类型黏弹材料制造的阻尼器在多种应变幅值、频率下的动态特性并与实验相比较,分析了黏弹阻尼器损耗模量、储能模量频变特性和双频激励对阻尼器的影响。结果表明,建立的非线性黏弹阻尼器动力学模型能够更好地反映不同类型黏弹材料构成的黏弹阻尼器的动刚度和阻尼,适合于直升机旋翼载荷计算和气动弹性分析。     

固体火箭发动机固有频率灵敏度特性的初步研究

本文运用固有频率灵敏度分析方法,把长细比较大发动机简化为梁模型,推导出其固有频率灵敏度计算公式;对于长细比较小发动机必需采用有限元模型,本文采用简化方法,进行固有频率灵敏度分析,并归纳出两种发动机的灵敏度特性.     

低雷诺数翼型和跨声速翼型边界层计算

本文利用边界层动量积分方程和平均流动能积分方程兼容计算了翼面的层流和湍流边界层流动。文中采用一种e~9型转捩判别公式预测翼面存在层流分离气泡情况的转捩位置。并引入对剪应力系数C_r的滞后方程以体现湍流中雷诺应力的历程效应。为避免在翼面流动分离时边界层方程的奇异,采用反解法计算。算例表明,计算与测量结果吻合良好。