Power-law spectra of energetic electrons in solar flares from the maximum entropy and dimensional considerations

The maximum entropy formalism and dimensional analysis are used to derive a power-law spectrum of accelerated electrons in impulsive solar flares, where the particles can contain a significant fraction of the total flare energy. Entropy considerations are used to derive a power-law spectrum for a particle distribution characterised by its order of magnitude of energy. The derivation extends an earlier one-dimensional argument to the case of an isotropic three-dimensional particle distribution. Dimensional arguments employ the idea that the spectrum should reflect a balance between the processes of energy input into the corona and energy dissipation in solar flares. The governing parameters are suggested on theoretical grounds and shown to be consistent with solar flare observations. The flare electron flux, differential in the non-relativistic electron kinetic energy E, is predicted to scale as $E^{-3}$. This scaling is in agreement with RHESSI measurements of the hard X-ray flux that is generated by deka-keV electrons, accelerated in intense solar flares.     

供电系统的干扰模式及抑制措施

供电系统的电磁干扰主要由发电机噪声、整流谐波、开关频率和它的谐波,以及在开关转换中高速电流和电压的瞬变所引起,这些干扰可通过传导和辐射的方式直接影响交流电网和用电设备。所以,本文所要讨论的主要问题就是电磁干扰的解决方法。     

几种新的单路原子磁导引磁场设计和分析

原子磁导引利用载流导线产生的磁场与原子相互作用来操控冷原子,针对冷原子操控和传输的要求,提出了双曲线薄板导引、双平行平板导引、三根等边三角形和四根正方形分布载流导线实现对冷原子进行单路磁导引的方案,利用Ansoft maxwell 2D软件计算各导引的磁场分布和沿特殊轴的磁场变化值,分析其导引特点。这几种磁导引都采用通直流电的载流导体,其结构中心位置的场强存在极小值,形成了沿着导引的方向呈现管状磁场分布,适合导引弱场搜寻态的原子。越接近导体表面的地方,磁场梯度越大,所以原子不易与材料的相互作用而被吸引到导体表面造成损耗,而且使用时不需另加控制磁场,在实验中易于实现。     

微小误差取舍准则的拓展及应用

介绍了微小误差取舍准则的定义和内容,并利用数学方法对准则进行了补充,使其在实际应用中更具操作性,同时对该准则在测量不确定度评定等领域的应用做了简要分析。     

Modeling and data analysis of a Forbush decrease

We study the Forbush decrease of the galactic cosmic ray intensity observed in 9–25 September 2005 using the experimental data and a newly developed time-dependent three dimensional modeling. We analyze neutron monitors and muon telescopes, and the interplanetary magnetic field data. We demonstrate a clear relationship between the rigidity (R) spectrum exponent (γ) of the Forbush decrease and the exponent (ν) of the power spectral density of the components of the interplanetary magnetic field in the frequency range of ∼ 10⁻⁶–10 ⁻⁵ Hz. We confirm that an inclusion of the time-dependent changes of the exponent ν makes the newly developed nonstationary three dimensional model of the Forbush decrease compatible with the experimental data. Also, we show that the changes of the rigidity spectrum exponent γ does not depend on the level of convection of the galactic cosmic rays stream by solar wind; depending on the changes of the exponent ν, i.e. on the state of the turbulence of the interplanetary magnetic field.     

泵浦光功率对核磁共振陀螺仪零偏的影响分析

核磁共振陀螺仪中,泵浦光频率和功率参量会对陀螺性能产生重要影响。研究了泵浦光功率对核磁共振陀螺仪零位的影响,阐明了不同谱线加宽条件下泵浦光功率稳定性与核磁共振陀螺仪零偏稳定性的关系。结果表明,泵浦光功率改变0.7‰,陀螺零位变化0.41(°)/s,且缓冲气体压强增大可以减小泵浦光功率对零位的影响。     

实心圆柱式永磁同步电机转子偏心气隙磁场的空间和频率特性

针对两极平行充磁实心圆柱式永磁同步电机(SCPMSM),分析转子偏心对气隙磁场空间和频率特性的影响。通过引入转子静态偏心和动态偏心磁导修正系数,建立了转子偏心气隙磁场的数学模型,分析了空载和负载情形下转子静态偏心以及动态偏心气隙磁场的空间和频率特性。以1台2极12槽SCPMSM为例,对转子偏心气隙磁场特性进行了有限元分析,验证了理论分析的正确性。     

火星车磁通门磁强计技术

火星磁场测量是国际火星探测任务的焦点之一,中国首次火星磁测任务通过在巡视器(即火星车)和环绕器上同时搭载磁强计,实现对火星磁场的火–空联合观测。巡视器磁强计载荷选用双探头三轴磁通门磁强计,采用亥姆霍兹补偿线圈型探头技术和全数字闭环反馈电路技术,实现空间磁场的高精度同点测量。单机在设计上考虑了可靠性安全性设计和空间环境适应性设计。经地面标定,单机量程可达到±6.5万nT,噪声水平优于0.01 nT/√Hz,分辨率达到了0.01 nT。     

同轴微阴极电弧推力器的粒子网格法数值模拟

采用粒子网格方法对同轴微阴极电弧推力器μCAT工作过程进行了模拟研究, 并应用自相似方法对模型进行简化,获得了推力器羽流区的电子数密度分布、离子数密度分布、电势分布及离子轴向平均速度,通过改变磁感应强度和位形分析磁场对推力器内等离子体运动特性及推力器性能的影响。计算结果表明,电子被外加磁场捕获约束在磁力线附近,低速离子与高速电子形成的双极扩散电场加速离子喷出;在相同流量情况下,磁感应强度002T时,离子返流严重,磁感应强度005~030T时,磁感应强度变化对速度影响较小;磁场位形对离子运动和推力器性能有较大影响,磁力线与轴线夹角较小时离子速度下降明显,夹角较大时离子返流严重。