Ulysses observations of latitude gradients in the heliospheric magnetic field: Radial component and variances

The radial component of the magnetic field at Ulysses, over latitudes from –10° to –45° and distances from 5.3 to 3.8 AU, compares very well with corresponding measurements being made by IMP-8 in the ecliptic at 1AU. There is little, if any, evidence of a latitude gradient. Variances in the field, normalized to the square of the field magnitude, show little change with latitude in variations in the magnitude but a large increase in the transverse field variations. The latter are shown to be caused by the presence of large amplitude, long period Alfvénic fluctuations. This identification is based on the close relation between the magnetic field and velocity perturbations including the effect of anisotropy in the solar wind pressure. The waves are propagating outward from the Sun, as in the ecliptic, but variance analysis indicates that the direction of propagation is radial rather than field-aligned. A significant long-period component of 10 hours is present.     

Ulysses out-of-ecliptic observations of “27-day” variations in high energy cosmic ray intensity

We report the discovery that for latitudes above 40°S, the observed recurring modulation of cosmic rays and anomalous nuclei occurs without the detection byUlysses of the solar wind velocity and magnetic field recurring enhancements that have, heretofore at lower latitudes, defined corotating interaction regions—i.e., the mechanism producing the recurring intensity variations >40°S appears to be located beyond the radial range ofUlysses.     

Interplanetary shock waves: Ulysses observations in and out of the ecliptic plane

Between its launch in October 1990 and the end of 1993, approximately 160 fast collisionless shock waves were observed in the solar wind by the Ulysses space probe. During the in-ecliptic part of the mission, to February 1992, the observed shock waves were first caused mainly by solar transient events following the solar maximum and the reorganisation of the large scale coronal fields. With the decay in solar activity, relatively stable Corotating Interaction Regions (CIRs) were observed betwen 3 and 5.4 AU, each associated with at least one forwardreverse shock pair. During the out-of-ecliptic phase of the orbit, from February 1992 onwards, CIRs and shock pairs associated with them continued to dominate the observations. From July 1992, Ulysses encountered the fast solar wind flow from the newly developed southern polar coronal hole, and from May 1993 remained in the unipolar magnetic region associated with this coronal hole. At latitudes beyond 30°, CIRs were associated almost exclusively with reverse shocks only. A comprehensive list of shock waves identified in the magnetic field and solar wind plasma data from Ulysses is given in Table 1. The principal characteristics were determined mainly from the magnetic field data. General considerations concerning the determination of shock characteristics are outlined in the Introduction.     

微型固体火箭发动机用短点火延迟点火器研究

短的点火延迟期对某些微型固体火箭发动机尤为重要。文中引用固相点火理论，在诸多向推进剂表面供热的方式中，着重分析了起重要作用的对流换热，认为提高点火燃气的流速能明显地提高点火燃气对推进剂表面的热交换率，使推进剂表面很快达到发火温度，在微型固体火箭发动机的短点火延迟点火器设计中应用了这一理论，并获得了理想的效果。     

固体火箭燃烧室内微粒分布的实验研究

介绍一种实时脉冲取样器用于测定固体火箭燃烧室内凝相微粒尺寸分布技术，实验结果表明，含铝推进剂微粒呈二模态或三模分布，燃烧室内压力大，微粒趋大，燃烧室压力很小，微粒亦趋大，有一最小尺寸的压力值，残渣影响微粒尺寸测量，而推进剂燃烧特性将直接影响着微粒尺寸分布。     

两种新型含铜催化剂对RDX／AP催化热分解的研究

通过热分解试验，系统地研究了两种新型含铜催化剂对ＲＤＸ，ＡＰ，ＲＤＸ／ＡＰ的催化作用，由热分析图谱及动力学计算结果可以看出：ＹＢ对ＡＰ，ＱＣ对ＲＤＸ及ＹＢ＋ＱＣ对ＲＤＸ／ＡＰ的热分解有明显的催化作用，其推进剂的燃速测定结果也进一步证明其催化效果。     

采用机械合金化工艺制备SiC质点弥散分布的Ti—6Al—4V复合粉末

对连续纤维增强和颗粒增强金属基复合材料的优缺点进行了评述。为制备ＳｉＣ质点弥散分布的Ｔｉ－６Ａｌ－４Ｖ复合粉末采用了机械合金化工艺技术。用ＸＲＤ和ＳＥＭ研究了机械合金化过程中粉末形貌、粒度和晶体结构的变化。     

热力系统中分布参数对象的数值─解析混合仿真方法

以热力系统中常见的管式换热器为对象，建立了包括质量、动量和能量平衡方程的集中参数数学模型，通过一系列的数值简化和处理，获得了能量方程的解析解，并发现此解的精度对时间步长的大小不很敏感。利用这一特性，本文提出了数值—解析混合仿真方法，采用多段集中参数模型同时选用较大的时间步长进行仿真。与非线性分布参数模型计算结果的对比表明，本仿真方法不仅具有较高的精度，同时也大大提高了计算速度，实现了仿真精度和实时性的统一。本方法对热力系统中分布参数对象的仿真具有重要意义。     

航空发动机实时寿命监视及数据处理方法研究

ＡＥＲＯＥＮＧＩＮＥＬＩＦＥＭＯＮＩＴＯＲＩＮＧＡＮＤＲＥＡＬ－ＴＩＭＥＤＡＴＡＰＲＯＣＥＳＳＩＮＧＨｅＪｉｎｇｌａｎ，ＨｏｎｇＪｉｅ，ＬｉＱｉｈａｎ（４ｔｈＤｅｐｔ．ＢｅｉｊｉｎｇＵｎｉｖｅｒｓｉｔｙｏｆＡｅｒｏｎａｕｔｉｃｓａｎｄＡｓｔｒｏｎａｕ...     

换热反问题输入数据的正则预处理及其对解的影响

ＲＥＧＵＬＡＲＩＺＡＴＩＯＮＰＲＯＣＥＳＳＩＮＧＯＦＩＮＰＵＴＤＡＴＡＩＮＩＮＶＥＲＳＥＨＥＡＴＴＲＡＮＳＦＥＲＰＲＯＢＬＥＭＡＮＤＩＴＳＩＮＦＬＵＥＮＣＥＯＮＴＨＥＳＯＬＵＴＩＯＮＺｈｏｕＪｉｎｇｗｅｉａｎｄＣｈｅｎｇＳｈａｎｇｍｏ（Ｄｅｐｔ．ｏｆ...