配置点谱方法求解非均匀介质内辐射传热问题

发动机内的燃气等高温介质随着组分和浓度的变化，会引起折射率在空间上的非均匀分布，从而导致辐射能束沿着曲线传播，其相应的辐射传热过程也更为复杂。为了避免射线追踪方法的复杂计算、提高计算效率，本文提出了配置点谱方法求解二维非均匀介质内辐射传热问题。在求解过程中，角向采用离散坐标法处理，空间采用配置点谱方法处理。通过将三种非均匀介质内辐射传热问题的配置点谱方法结果与文献结果进行对比分析，发现配置点谱方法可以在较少的节点数下，获得准确、有效地计算结果。并且，采用配置点谱方法求解三种算例的计算时间均消耗较少，均在20分钟以内。这将为进一步开展发动机复杂结构内高温燃气辐射快速仿真提供基础。     

半透明吸收、散射性介质内辐射传递系数的新型计算方法

为考虑半透明吸收、散射性介质内各向同性散射对辐射能量传递过程的影响，通过对辐射能量传递过程的分解，提出了一种基于辐射能量传递过程分解的射线踪迹法，该计算方法无需引入预设控制精度参数。经与其他计算方法的比较表明，该新型计算方法正确，计算精度高、计算时间短，可以用于研究介质内辐射能量传递过程的研究。     

On the correlation of the solar wind observed at the L5 point and at the Earth

The L5 point is a promising location for forecasting co-rotating high-speed streams in the solar wind arriving at the Earth. We correlated the solar wind data obtained by the Nozomi spacecraft in interplanetary space and by the Advanced Composition Explorer (ACE) at the L1 point, and found that the correlation is significantly improved from that of the 27-day recurrence of ACE data. Based on the correlation between the two spacecraft observations, we estimated the correlation of the solar wind velocity between the L5 point and at the Earth, and found that the correlation coefficient was about 0.78 in late 1999, while that of the 27-day recurrence was 0.51. Eighty-eight percent of the velocity difference falls within 100 km/s between the L5 point and the Earth. This demonstrates the potential capability of solar wind monitoring at the L5 point to forecast the geomagnetic disturbances 4.5 days in advance.     

多元系统论视角下的中国文化与美国诗歌

自19世纪以来中国诗歌的英译对美国诗歌产生了重大影响,但美国本土诗歌和文化思想仍然处于强势的主导地位,美国人接受的是他们心目中的中国文化。美国诗歌对中国文化和中国诗歌的吸收,并不等于东西文化的交流与结合。通过研究中美文化和文学交流的媒介,结合多元系统论和比较文学相关理论来对该问题进行分析。     

Interplanetary medium – A dusty plasma

The average mass of dust per volume in space equals that of the solar wind so that the interplanetary medium should provide an obvious region to study dust plasma interactions. While dust collective behavior is typically not observed in the interplanetary medium, the dust component rather consists of isolated grains screened by and interacting with the plasma. Space measurements have revealed several phenomena possibly resulting from dust plasma interactions, but most of the dust plasma interactions are at present not quantified. Examples are the production of neutrals and pick-up ions from the dust, dust impact generated field variations at spacecraft and magnetic field variations possibly caused by solar wind interacting with dust trails. Since dust particles carry a surface charge, they are exposed to the Lorentz force in the interplanetary magnetic field and for grains of sub-micrometer sizes acceleration can be substantial.     

高压高扬程固液两相介质离心泵的设计原则

固液两相介质离心泵主要用于煤化工、冶金、电力、石油化工、市政工程等领域,用于输送含灰渣、固体杂质和浆体的介质,其扬程一般不超过80m。超过80m扬程的高压高扬程固液两相介质离心泵可以用作煤气化工业中的激冷水泵、洗涤塔循环泵和石化行业PTA装置中的TA浆料供料泵,在这类泵的设计中有些需要特别关注的技术特点。从转子刚性、轴向力平衡、过流部件设计的适用性、支撑系统的稳定性、机械密封设计的可靠性等几个方面论述了高压高扬程固液两相介质离心泵的设计原则。     

Cosmic ray flux at the Earth in a variable heliosphere

In recent years the variability of the cosmic ray flux has become one of the main issues not only for the interpretation of the abundances of cosmogenic isotopes in cosmochronic archives like, e.g., ice cores, but also for its potential impact on the terrestrial climate. It has been re-emphasized that the cosmic ray flux is not only varying due to the solar activity-induced changes of the solar wind but also in response to the changing state of the interstellar medium surrounding the heliosphere. We demonstrate the significance of these external boundary condition changes along the galactic orbit of the Sun for the flux as well as spectra of cosmic rays. Such interstellar–terrestrial relations are a major topic of the International Heliophysical Year 2007.     

MHD modeling of the outer heliosphere: Achievements and challenges

An overview is presented of magnetic-field-related effects in the solar wind (SW) interaction with the local interstellar medium (LISM) and the different theoretical approaches used in their investigation. We discuss the possibility that the interstellar magnetic field (ISMF) introduces north–south and east–west asymmetries of the heliosphere, which might explain observational data obtained by the Voyager 1 and Voyager 2 spacecraft. The SW–LISM interaction parameters that are responsible for the deflection of the interstellar neutral hydrogen flow from the direction of propagation of neutral helium in the inner heliosheath are outlined. The possibility of a strong ISMF, which increases the heliospheric asymmetry and the H–He flow deflection, is discussed. The effect of the combination of a slow-fast solar wind during solar minimum over the Sun’s 11-year activity cycle is illustrated. The consequences of a tilt between the Sun’s magnetic and rotational axes are analyzed. Band-like areas of an increased magnetic field distribution in the outer heliosheath are sought in order to discover regions of possible 2–3 kHz radio emission.     

First millimetric detections of AE Aquarii

We report the first millimetric detections of the magnetic cataclysmic variable AE Aquarii, accompanied by contemporaneous microwave observations. These data show that the time-averaged spectrum is well fit by a power-law which extends to mm wavelengths. We suggest that the spectrum is consistent with that expected from a superposition of flare-like events.     

MANET中一种新的基于多包接收的媒体接入控制协议

提出了一种新的基于多包接收的MANET媒体接入控制协议.该协议利用信道多包接收的特性,结合功率控制和协议的跨层设计,可选取信道增益较大的节点接入信道.实验结果表明,在业务量较大时,新协议在提高网络吞吐量的同时,减小了能量消耗.