高密度喷气燃料与常规喷气燃料浓度场试验研究

本文利用ＣＯ２红外气体分析仪和取样管对高密度喷燃料和常规喷气燃料在直流喷嘴下游的浓度场分布进行了测量，就气流速度，油压降和下游距离对浓度场分布的影响进行了对比研究。试验结果表明，在相同工况下，常规喷气燃料的最大浓度值比高密度喷气燃料的大；气流速度和油压变化对高密度喷气燃料最大浓度点穿透深度的影响大于对常规喷气燃料的影响。     

Avoid online radiation risk: Theoretical simulation of chromosome breaks in cells exposed to heavy ions

In this study, we report an easy and quick method on simulating chromosome breaks in cells exposed to heavy charged particles. The theoretical value of chromosome break was calculated, and validated comparison with experimental value by using premature chromosome condensation technique. A good consistency was found between theoretical and experimental value. This suggested that higher relative biological effectiveness of heavy ions was closely correlated with its physical characteristics. Also, a safe approach on predicting chromosome breaks in cells exposed to heavy ions at off-line environment can be considered. Furthermore, three key factors influencing the theoretical simulation was investigated and discussed.     

重金属复合污染红壤增施石灰石对黑麦草生长的影响

利用两种剂量石灰石改良受重金属复合污染红壤的理化性质，使其PH值分别提高到4．67—4．93和6．19—6．73的范围。测定一年生黑麦草的生物量、重金属含量及土壤中重金属有效态含量，对黑麦草—土壤系统中重金属含量进行相关分析。实验说明，污染红壤增施石灰石能改善黑麦草的生长，当土壤PH值达6．0以上时，黑麦草的生长情况更好。有效态离子冲量是一种表征黑麦草—土壤中重金属含量的良好方法。     

大连机场一次罕见的连续四天大雾低云过程分析

本文利用常规天气图、探空图和三维中尺度模式,对大连机场2011年6月29日到7月3日出现的连续4天的大雾低云天气进行分析,发现此次大雾低云过程发生同副热带高压的位置和强度变化密不可分:副热带高压中高层的下沉逆温对大雾低云天气的低层稳定层的产生和维持起到重要作用;同时它的西进北抬和东撤南退直接导致大连机场上游天气系统三次槽线东移,进而影响本场。近地面层的水汽辐合和弱冷暖气流交汇为大雾低云天气得以维持提供良好的水汽条件。     

载人登月运载火箭总体方案研究

介绍了国外重型运载火箭方案技术特点和性能,对我国新一代运载火箭发动机研制给出了以两级半构型为重型运载首选、120,400t推力吨位可满足我国未来运载火箭一级动力需求、100t级真空推力氢氧发动机是我国重型运载较佳选择,以及箭体直径最大7～8m为宜的建议。针对我国的载人登月任务,提出了重型运载的四条发展路线,优选了一型运载火箭并进行了细化设计。     

On kinematics of gas clouds in the broad-line region of active galactic nuclei and quasars

The kinematics of gas clouds in broad-line region of active galactic nuclei and quasars is considered. The motion of the clouds is governed by three forces — gravitational influence from the central supermassive body, radiational pressure from the continuum radiation, and resistance of the intercloud medium. Clouds moves radial but only outward motion gives a velocity field, which is in accordance with the observational data. The profiles of the permited lines are obtained in some simplify assumptions for the emissive capacity of the gas in clouds, and are in good agreement with the observational data. In the framework of the model under consideration there is a possibility to estimate some physical parameters of the nuclei such as mass of the central body and density of the intercloud medium.     

RATAN-600 and RadioAstron reveal the neutrino-associated blazar TXS 0506+056 as a typical variable AGN

The possible association with the high-energy neutrino event IceCube-170922A has sparked interest in the blazar TXS 0506+056. We present 72 instantaneous 1–22 GHz spectra measured over the past 20 years with the RATAN-600 telescope and compare them with the results of observations of 700 variable Active Galactic Nuclei (AGN) studied within the same program. The recent radio flare of TXS 0506+056 started from a minimum in 2013 and reached its first peak in December 2017 and a second peak in May-June 2018. This was the third strong radio flare in this source since 1997. The spectrum remains nearly flat during the flares. The spectral shape and variability pattern observed in TXS 0506+056 are typical for variable AGN. RadioAstron Space VLBI observations in 2013–2015 did not detect TXS 0506+056 on space-ground baselines of more than 9 Earth diameters. However, an observation on 23 September 2015 resulted in the detection of interferometric signal on 6 Earth diameter baselines at 18 cm close to the detection limit. We consider the possibility that TXS 0506+056 and other AGN may accelerate relativistic protons more efficiently than electrons. Relativistic protons are necessary to produce both the high-energy neutrinos observed in the IceCube Observatory and the high AGN brightness temperatures implied by the RadioAstron detection. They may also provide the main contribution to the observed synchrotron radiation of parsec-scale AGN jets. This supports the suggestion that relativistic protons may play a much more important part in extragalactic astrophysics than earlier anticipated.     

网络分析仪法测量稠油介电常数

用网络分析仪在Ｘ波段８～１１．５ＧＨｚ的６个频率点上,对大港、胜利、辽河油田稠油的介电常数进行测量,测量结果可以为微波采油工艺中的井下轴射器的设计及微波能利用率的估算提供理论依据,并对测量结果进行了误差分析。     

Status of the Hard X-ray Modulation Telescope Project

The Hard X-ray Modulation Telescope (HXMT) is China's first astronomical satellite. It will perform a broad band (1-250keV) scan survey and do pointed observations of X-ray sources to study their spectra and multi-wavelength temporal properties. The pre-flight models of the satellites have been finished, and the flight models are in production. The expected launch date of HXMT is in late 2015.