On the origin of cosmic rays in the spiral galaxy NGC 3310

The problem of cosmic ray production in the spiral galaxy NGC 3310 is addressed by analysing and comparing optical and radio continuum data. Tentative results indicate that on global scales relativistic electrons may be produced in the shock front associated with teh density wave while on local scales extreme population I objects may be producing them. It is inferred that the same conclusions apply to all cosmic rays produced in the disk.     

架空线自阻尼的测试方法

自阻尼是导线的基本特性之一。在高压架空导线防振设计中,自阻尼是一个基础数据。本文是介绍对导线自阻尼的三种测试方法。其中的“剪力法”是我们自己研创的新方法。文中不仅介绍了测量技术,还附有在我国第一次测出的 LGJQ-400型导线的自阻尼数据。     

超临界正癸烷同轴剪切喷注热声振荡数值模拟

以液体火箭发动机同轴剪切喷嘴燃烧室作为研究对象,对超临界压力下低温正癸烷向高温正癸烷喷注过程中,由于高温正癸烷被快速冷却导致密度剧烈变化进而引发的热声振荡现象进行数值模拟。研究了出口压力、高温正癸烷流动速度与温度、低温正癸烷喷注速度与温度对热声波振幅与频率的影响。结果表明：当高温正癸烷被快速冷却时,其自身体积快速收缩,同时由于附近高温正癸烷的惯性导致压力先增大后减小,快速交替变化,从而产生热声波在高温正癸烷中传播。热声波振幅与频率的大小主要由高温正癸烷在不同压力与温度下的热物性决定。热声波的频率随着高温正癸烷声速增大而增大;热声波的振幅由高温正癸烷的相对压力系数与温度变化率共同决定。     

色散和耗散对Alfven孤立波的影响

利用变数变换和解析积分的方法,分别找到了带色散项的DNLS方程和带耗散的MKdV方程的一类解析解,给出了存在孤立波的条件。      

反向电集流出现率与大气准两年振荡

本文分析印度Trivandrum地磁台的约两个太阳黑子周期的地磁场水平分量小时值。在部分地消除了太阳黑子周期及一年周期变化后,发现了反向电集流出现率的QBO调制现象:QBO东风相反向电集流出现率增加;QBO西风相反向电集流出现率减小。据此讨论了反向电集流的形成机制,认为大气行星波在其上传过程中与太阳半日波或太阴半日波的相互作用,有可能导致两种半日波的放大和相位移动,并最终导致反向电集流的出现。      

A REPORT OF GROUND EXPERIMENTS FOR BRAIN FUNCTION IN SPACE

The brain function is of crucial importance in space adaptation and astronaut performance. According to the theory of nonequiliblium fluctuations a new technology, ET (Elec-troencephalofluctuography [EEFG] Technology), has been developed in our laboratory for space application. Information of different attracters, especially the dominant supra-slow (S) oscillations of the brain can be abstracted from the fluctuating brain waves. Specific Sspectral lines related to neurophysiological and neuro-chemical activities have been identified and charcteristic spatial patterns have been figured out. ETanalysis has been carried out in a series of ground experiments: (1) 20 degrees head lowered suspension experiments in rabbits; (2) 2Gz hypergravity experiments in rabbits; (3) effects of antimotionsickness drugs on rabbits during suspension; (4) clincal observations on patients with brain circulation diseases. Valuable information has been collected in all these experiments, which can hardly be obtained by means of other existing techniques. The potentiality of ETapplication in space research was discussed.      

激光引致水诱导空气击穿所获无约束流场演化过程的实验研究

流场演化过程是揭示激光推进机理的重要研究内容之一。利用纹影系统和PCO-HSFC 高速相机,首次拍摄了自来水诱导CO₂激光击穿空气产生的激波向空气和水中的演化过程。阐述了产生两次气蚀空穴的原因：初始时刻产生的空穴为激波作用于水面所致,第二次空穴出现在相机被触发后约8 μs 时,是激光烧蚀水蒸气作用于水面所形成的低压区。实验结果表明：击穿后流场向激光入射方向（空气中）演化较快,激波初速度较大,约为6 km/s;流场向水中演化相对较缓,激波初速度约为3.33 km/s。两者都服从指数衰减,分别在约73.368 μs 和41.649 μs 时衰减到声速。研究结果对于把水作为工质应用于激光推进有一定意义。     

Polarization pattern of low and mid-frequency magnetic pulsations in the polar cap: A comprehensive analysis at Terra Nova Bay (Antarctica)

The polarization pattern of ULF pulsations (f ≈ 1–100 mHz) at Terra Nova Bay (Antarctica, CGM λ ∼ 80°) has been determined for the entire 2003, soon after the solar maximum. A comparison with the results of previous investigations, conducted at the same station close to the solar minimum (1994–96), allows to focus common elements and major differences among different frequency bands which persist through the entire solar cycle. Basically, between f ∼ 1.5 and 5 mHz, the day can be divided into four sectors with alternate polarizations. The local time and latitudinal dependence of the observed pattern can be tentatively interpreted in terms of a latitude of resonant field lines reaching λ ∼ 80° in the noon sector; on the other hand, resonance effects of lower latitude field lines can be clearly identified also far from the noon meridian when the station moves into the deep polar cap. Moreover, in the morning sector the resonance region would extend to lower latitudes than in the evening sector. The proposed profile of the resonant region can interpret also the results obtained at other cusp/auroral stations and appears consistent with that one inferred in the northern hemisphere at smaller latitudes. The resonance region progressively shifts toward lower latitude with increasing frequency; correspondingly, the four-sector pattern progressively disappears at TNB. Above f ∼ 20 mHz, the experimental observations might suggest an additional contribution from Sunward propagating waves, possibly via the magnetotail lobes.     

Ionospheric oscillations caused by geomagnetic Pi2 pulsations and their observations by multipoint continuous Doppler sounding; first results

In 2004, we started operating a continuous Doppler sounding system to investigate ionospheric signatures of infrasonic, short period acoustic gravity waves and geomagnetic pulsations. Since January 2007, four stable 3.59 MHz transmitters have been in operation in the western part of the Czech Republic. Multipoint measurements enable us to investigate horizontal propagation of waves and disturbances in the ionosphere and to estimate horizontal distances over which these waves (disturbances) are correlated.