航天记录器的发展和转型

概述中国航天记录器近五十年的发展历程,阐述航天记录器技术转型的十年过程,简要介绍目前航天记录器应用的新进展。     

Upper limit of the total magnetic flux in an active region according to the photometric-magnetic dynamical model

The photometric-magnetic dynamical model handles the evolution of an individual sunspot as an autonomous nonlinear, though integrable, dynamical system. One of its consequences is the prediction of an upper limit of the sunspot areas. This upper limit is analytically expressed by the model parameters, while its calculated value is verified by the observational data. In addition, an upper limit for the magnetic strength inside the sunspot is also predicted, and then, we obtain the following significant result: The upper limit of the total magnetic flux in an active region is found to be of about 7.23 × 10²³ Mx, namely, phenomenologically equal to the magnetic flux concentrated in the totality of the granules of the quiet Sun, having a typical maximum magnetic strength of about 12G. Therefore, the magnetic flux concentrated in an active region cannot exceed the magnetic flux concentrated in the photosphere as a whole.     

Modelling and observations of photospheric magnetic helicity

Mounting observational evidence of the emergence of twisted magnetic flux tubes through the photosphere have now been published. Such flux tubes, formed by the solar dynamo and transported through the convection zone, eventually reach the solar atmosphere. Their accumulation in the solar corona leads to flares and coronal mass ejections. Since reconnections occur during the evolution of the flux tubes, the concepts of twist and magnetic stress become inappropriate. Magnetic helicity, as a well preserved quantity, in particular in plasma with high magnetic Reynolds number, is a more suitable physical quantity to use, even if reconnection is involved.     

小型磁偏转质谱计性能实验研究

自主研发了小型磁偏转质谱计,并对其质量范围、分辨本领、灵敏度和最小可检分压力四个主要性能指标进行了实验测试和比对。结果表明,该质谱计的质量范围为（1~143）amu,相对N₂的分辨本领为1400,灵敏度为4.2×10^-5 A/Pa,最小可检分压力为9.5×10^-7 Pa。该测试和比对结果为磁偏转质谱计进一步的优化设计和性能提高奠定了重要基础。     

(70~100)MeV准单能中子参考辐射场设计

国内基于串列加速器建立了144keV~15MeV的单能中子参考辐射场,解决了20MeV以下能区中子探测器注量、剂量等参数的量值溯源,但尚未建立20MeV以上能区准单能中子参考辐射场。随着航天空间中子探测任务的需要以及地面高能质子加速器的发展,20MeV以上能区准单能中子参考辐射场需求越来越突出。发展20MeV以上能区高能中子参考辐射场对于满足国防需求、推动中子计量学科发展具有重要意义。     

Ionospheric parameters in the European sector during the magnetic storm of August 25–26, 2018

Variations of ionospheric parameters Total Electron Content (TEC) by GNSS, critical frequency (foF2) by vertical sounding and electron density (Ne) by low-altitude satellite were studied at high, mid and low latitudes of the European sector during the magnetic storm of August 25–26, 2018. During the main phase of the storm the ionospheric F2-layer was under the positive disturbance at mid and low latitudes. Then the transition from the positive to negative ΔfoF2 values occurred at all latitudes. The recovery phase was characterized by negative ionospheric disturbance at all latitudes. This is due to the decrease of thermospheric O/N2 ratio during the recovery phase of the storm. The intense Es layers screened the reflections from the F2-layer on August 26th at high and at low latitudes but at different times. Some blackouts occurred due to the high absorption level at high latitudes. In general, foF2 and TEC data were highly correlated. The major Ne changes were at the low latitudes. In general, Ne data confirmed the ionospheric dynamics revealed with foF2 and TEC.     

三维非线性撕裂模耦合和快速磁场重联

基于三维不可压缩电阻性ＭＨＤ方程，在长柱形位型下，数值研究了电阻撕裂模不稳定性所引起的磁场重联过程。研究结果表明，撕裂模的非线性相互作用和耦合，将产生许多模式的强裂解稳和导致快速的磁场重联。这一过程的进一步发展，导致具有螺旋形结构，不同模式的磁岛磁力线重叠，从而引起较大区域内的磁场各态经历和磁力线随机走向，形成撕裂模端动。     

电脑控制磁粉探伤机的研制

本文介绍了利用ＭＣＳ－５１单片机进行磁化参数与操作功能控制的磁粉探伤的工作原理，特点及技术性能。该机经民航，汽车等知业检验部门的使用效果良好。     

多项式系统几何性质的注记

证明：在研究多项式系统的几何性质时，多项式系统应当定义成射影空间中奇点集之余维数至少为2的线场。在这个定义中，多项式系统的次数与通常的次数，在概念上不同相同，通常的n 1次退化系统属于这里的n次系统。值得注意的是，本给出的定义与坐标系的选取无关，在这种定义下，多项式系统的某些几何性质变得非常明显。     

码分复用系统的纠错码

依据有限域直和与有限环同构的代数性质，对多路复用系统构造线性分组码。其特点是既实现码分复用，又具有纠错能力，提高系统的传输可靠性。合路器是一种同构映射运算，将ｍ路有限域上的线性分组码唯一地映射成有限环上的单一码字，实现在宽带信道上同时传输ｍ路数据。收端经逆映射完成分路，一旦发生信道传输错误时，译码器在各码纠错能力范围内实现纠错。文中叙述了复用系统线性分组码的编译码方法，给出了同构映射运算的算法。