X射线耀斑的强度指标

本文利用GOES-7卫星的1分钟记录资料研究了1991年3月和6月期间6个大X耀斑伴随的软X射线爆发特性和源强度的关系。结果指出：对X射线耀斑，其射线辐射流量上升快的在日冕中激起的激波速度也较快．数值模拟研究指出，这可能反映爆发能量释放速率是源强度的主要指标．     

Response of the low latitude geomagnetic field to the major proton event of November 2001

A major solar flare eruption occurred at 16:20 UT on 4 November 2001, followed by strong solar radiation storm and proton event recorded by the SOHO and other interplanetary satellites. Coronal mass ejection associated with the flare event triggered an interplanetary shock, which impacted the geomagnetic field after about 33 h. The shock impact was quite intense to produce a SSC magnitude of 80 nT in the low latitude ground magnetic records followed by sharp and deep main phase (Dst −300 nT) in the first stage, following the density (N_p) enhancement. High time resolution digital magnetic field data from the equatorial and low latitude stations in India are analyzed to study the influence of various IP parameters on the intensity and duration of the magnetic storm. A double step storm was found to be in progress caused by the multiple injections. During the period of recovery, after a period of 8 h, a third stage of depression in the ground magnetic field was set in, which corresponded to the southward directed Bz. The energy transfer processes associated with the event is presented.     

小推力单元肼推力器温度场数值分析 （I）实验验证和保温套筒对温度场影响探析

建立了某小推力单组元肼推力器的全仿真传热数学模型，应用有限元分析方法对长程工作的不带套筒推力器瞬态温度场进行了热分析计算，并与试车温度数据进行了比较，数值计算结果与实验结果吻合良好，证明所用软件建立的模型合理。对增加套筒后的推力器进行了仿真模拟，结果表明，推力器脉冲长程工作后，单层套筒点焊于法兰盘上时集液腔温度较高，双层套筒时集液腔温度最高，均对法兰盘集液腔及电磁阀产生高温不利影响，推荐使用点焊在热控环上的热控方式；推力器温启动时，单、双层套筒保温效果相差不大，推荐使用单层套筒点焊于热控环上的热控方式。     

1991年6月地磁扰动—地面和同步高度特征

给出了1991年6月地磁扰动的地面和同步高度特征及引起这些扰动的可能的源.在长达近对天的扰动过程中，出现四次主相强度不同的磁暴和多次强急始，有的磁暴由多次扰动迭加而形成形态复杂的复合型磁暴·同步高度Hq分量多次出现反相.这些特征很可能主要是对广大的行星际空间多个高速度高密度结构的响应，这些结构有时伴随大尺度强南向磁场分量.     

某刹车装置的活塞组件衬套裂纹机理探究

某刹车装置耐久性试验中,活塞组件的衬套出现疲劳裂纹,经分析是由于汽缸座和刹车壳体外翘,活塞在与刹车盘间的摩擦力作用下对衬套外端产生交变挤压所致,试验验证结果成立,证明产品刚性影响构件的疲劳寿命。     

Solar Radio Bursts with Drifting Stripes in Emission and Absorption

This review covers fairly comprehensively experimental and theoretical research on the fine structure of types zebra pattern (ZP) and fiber bursts (FB) in solar type II + IV radio bursts. The basic attention is given to the latest experimental data. A comparative analysis of several recent solar type IV radio outbursts with these fine structure in dynamical radio spectra is carried out using available ground-based and satellite data (Yohkoh, SOHO, TRACE, RHESSI). New data on microwave zebra structures and fiber bursts testifies that they are analogous to similar structures observed at meter wavelengths. The discovery of the superfine structure, in the form of millisecond spikes is the most significant new effect in the cm range. All basic theoretical models of the zebra pattern and fiber bursts are discussed critically. Two main models are studied for their interpretation: (i) interactions between electrostatic plasma waves and whistlers, (ii) radio emission at double plasma resonance (DPR). The relative significance of several possible mechanisms remains uncertain.     

Relativistic proton production at the Sun in the 20 January 2005 solar event

Based on the concept of multiple acceleration of solar energetic particles (SEP) we analyzed the super-event of 20 January 2005 by the data of ground level, balloon and spacecraft observations. The main characteristics of relativistic solar protons (energy spectra, anisotropy directions and pitch-angle distributions) are derived and their dynamics during the event is studied. It is shown that the flux of relativistic solar protons may consist of two distinct components, the so-called prompt and delayed ones. Within a two-source model of particle generation, one of which is associated with an expanding magnetic loop, we solved the transport equation in energy phase space, including adiabatic losses simultaneously with the stochastic acceleration process, and calculate the expected spectra of the delayed component at the source. The confrontation of experimental spectra with theoretical ones shows that the delayed component may be correctly described by stochastic acceleration, but not the prompt component. The required acceleration efficiencies turned out to be rather high, so that, for this particular event, adiabatic cooling is practically negligible. Our results provide a new support to the existence of two populations of relativistic solar protons in some SEP events.     

Ionospheric storm of September 2017 observed at ionospheric station Pruhonice,the Czech Republic

The ionospheric effects induced by the September 2017 storm have been exceptional compared to other events in the solar cycle 24. This paper gathers results of the ionospheric observations at the European middle latitude station Pruhonice. It consists of evaluation of ionospheric vertical and oblique sounding, Digisonde drift measurement, and data obtained from the Continuous Doppler Sounding System. We observed strong ionospheric response with an unusual stratification of ionospheric layers, Large Scale Traveling ionospheric disturbances, changes in electron density, and increase and oscillations in plasma drift velocity.     

气冷喷油杆隔热套高度对混合扩压器性能影响

针对一种带气冷喷油杆的混合扩压器,基于Navier-Stokes方程组建立了流场三维数值计算模型,研究了气冷喷油杆的隔热套高度对一体化混合扩压器流场、流阻特性和混合特性的气动热力性能影响规律。结果表明:隔热套高度对混合扩压器热混合效率影响不大,总体变化范围小于0.008;随着隔热套高度的增加,静压恢复系数逐渐减小,流阻系数和压力损失系数逐渐增大;在混合扩压器出口截面处,总压恢复系数随隔热套高度增加而逐渐减小,且总体变化范围较小,由0.991 1减小到0.990 7。      

1980年11月6日—7日耀斑后冕拱的激活机制

1980年11月6日耀斑后冕拱(Post-flare coronal arch)在母耀斑(AR2779)开始后3小时形成, 并在形成后11小时和25小时两次激活。两次激活均由双带耀斑的增长环系所致。本文提出了激波加热和Petschek重连是该冕拱有效的激活机制。导出并求解了考虑辐射损失、热传导、激波加热和Petschek重连加热的冕拱能量方程。理论计算结果与Svestka根据SMM空间资料所给出的该冕拱的激活曲线基本符合。