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251.
252.
研究了主动电磁轴承支承的单盘柔性转子系统在磁轴承失效后转子坠落在带有固定间隙的滚动型备用轴承上的瞬态响应,分析了备用轴承的各种参数对瞬态响应的影响。结果发现系统出现了以自由落体-碰撞弹起-自由落体为特征的在间隙圆底部的摆动运动、以碰撞弹起-加速落体-碰撞弹起为特征的在整个间隙圆范围的碰撞型回转运动以及轴颈与备用轴承始终接触在一起的摩擦型回转运动等3种运动形式。碰撞型回转运动实际上是由碰撞过程中部分周向的摩碰引起,而摩擦型回转运动是由轴颈与备用轴承之间的全周干摩擦所致。碰撞型回转运动和反向摩擦型回转运动对备用轴承的影响最为严重。 相似文献
253.
磁悬浮轴承柔性转子系统的转速范围较大,固定的控制参数很难同时保证系统所需的低频和高频特性。本文在一般单神经元PID控制的基础上,将转速信号引入磁悬浮轴承数字控制器,在不同转速段选择不同的学习速率以调节控制参数得到合适的磁悬浮轴承的刚度和阻尼。试验结果表明,变学习速率单神经元自适应PID控制能够明显减小转子在各阶临界转速时的振幅,有助于磁悬浮轴承柔性转子系统的安全稳定运行。 相似文献
254.
用基于密度泛函理论的第一性原理方法,系统地研究了压力对Fe16N2体系结构和磁性的影响。结果表明仅仅离N位最远的Fe Ⅲ拥有一个约为2.84μB的大磁矩,而FeⅠ和Fe Ⅱ原子没有大磁矩产生。此外,还发现从0到47 GPa,总磁矩和单胞体积随着压力的增加单调减小,然而,在48 GPa的压力作用下,伴随着单胞体积的剧减,体系总磁矩消失。 相似文献
255.
依据经典的磁探仪应召搜潜方法,以某型反潜巡逻机为背景,建立了反潜巡逻机利用磁探仪执行平行航线、扩展矩形和螺旋形搜潜模型.对3种方法的搜潜概率进行分析,仿真了相同潜艇运动模型条件下,潜艇初始位置散布、初始距离、潜艇经济航速和海洋环境磁噪声对搜潜概率的影响.实验结果表明:相同条件下,螺旋形搜潜效能最高;潜艇只进行航速机动时... 相似文献
256.
为了研究冷原子在磁导引中的运动规律,设计优化导体结构、电流和偏置磁场,本文根据毕奥-萨伐尔定律计算理想化导体的常规数值解,并由Matlab和VC混合编程设计出导线磁场计算工具;根据麦克斯韦方程组选择Ansoft MaxweU计算宽导线、复杂结构导体、通交变电流等情况的有限元数值解.取宽度为100μm,高度为10μm的宽... 相似文献
257.
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. 相似文献
258.
Cool giant and supergiant stars generally present low velocity winds with high mass-loss rates. Several models have been proposed
to explain the acceleration process of these winds. Although dust is known to be present in these objects, the radiation pressure
on these particles is uneffective in reproducing the observed physical parameters of the wind. The most promising acceleration
mechanism cited in the literature is the transference of momentum and energy from Alfvén waves to the gas. Usually, these
models consider the wind to be isothermal. We present a stellar wind model in which the Alfvén waves are used as the main
acceleration mechanism, and determine the temperature profile by solving the energy equation taking into account both the
radiative losses and the wave heating. We also determine, self-consistently, the magnetic field geometry as the result of
the competition between the magnetic field and the thermal pressure gradient. As the main result, we show that the magnetic
geometry presents a super-radial index in the region where the gas pressure is increasing. However, this super-radial index
is greater than that observed for the solar corona. 相似文献
259.
通过分析高频磁场作用下熔体连续处理时夹杂的去除效率表明,熔体连续处理条件下的夹杂去除效率比熔体静止时的略低,而夹杂与熔体之间的密度差对电磁分离时的去除效率影响不大。提高去除效率的有效途径是增大磁感应强度或降低分离器管径,但减小管径的同时需要提高磁场频率,以保持α/δ的值在2附近才可以取得最佳的分离效果。 相似文献
260.