Geoeffectivity of Coronal Mass Ejections

Coronal mass ejections and post-shock streams driven by them are the most efficient drivers of strong magnetospheric activity, magnetic storms. For this reason there is considerable interest in trying to make reliable forecasts for the effects of CMEs as much in advance as possible. To succeed this requires understanding of all aspects related to CMEs, starting from their emergence on the Sun to their propagation to the vicinity of the Earth and to effects within the magnetosphere. In this article we discuss some recent results on the geoeffectivity of different types of CME/shock structures. A particularly intriguing observation is that smoothly rotating magnetic fields within CMEs are most efficient in driving storm activity seen in the inner magnetosphere due to enhanced ring current, whereas the sheath regions between the shock and the ejecta tend to favour high-latitude activity.     

Solar Sources of Heliospheric Energetic Electron Events—Shocks or Flares?

Electrons with near-relativistic (E≳30 keV, NrR) and relativistic (E≳0.3 MeV) energies are often observed as discrete events in the inner heliosphere following solar transient activity. Several acceleration mechanisms have been proposed for the production of those electrons. One candidate is acceleration at MHD shocks driven by coronal mass ejections (CMEs) with speeds ≳1000 km s⁻¹. Many NrR electron events are temporally associated only with flares while others are associated with flares as well as with CMEs or with radio type II shock waves. Since CME onsets and associated flares are roughly simultaneous, distinguishing the sources of electron events is a serious challenge. On a phenomenological basis two classes of solar electron events were known several decades ago, but recent observations have presented a more complex picture. We review early and recent observational results to deduce different electron event classes and their viable acceleration mechanisms, defined broadly as shocks versus flares. The NrR and relativistic electrons are treated separately. Topics covered are: solar electron injection delays from flare impulsive phases; comparisons of electron intensities and spectra with flares, CMEs and accompanying solar energetic proton (SEP) events; multiple spacecraft observations; two-phase electron events; coronal flares; shock-associated (SA) events; electron spectral invariance; and solar electron intensity size distributions. This evidence suggests that CME-driven shocks are statistically the dominant acceleration mechanism of relativistic events, but most NrR electron events result from flares. Determining the solar origin of a given NrR or relativistic electron event remains a difficult proposition, and suggestions for future work are given.     

高温下DD6单晶气冷叶片模拟试样拉伸性能试验

通过选晶法制备DD6单晶薄壁圆管模拟试样,对850℃和980℃两种温度下[001]晶体取向含与不含气膜孔的薄壁试管进行拉伸性能试验研究.结果表明:在850℃条件下,[001]取向含气膜孔的拉伸性能比[001]取向不含气膜孔的拉伸性能降低10.5%;在980℃条件下,[001]取向含气膜孔的拉伸性能与[001]取向不含气膜孔的拉伸性能水平相当,这表明温度越高,气膜孔对薄壁件拉伸性能的影响越不显著;但在980℃ 条件下,[001]取向通气状态的拉伸强度比不通气状态下的拉伸强度提高16%.同时,发现圆管表面状态及通气状态是影响单晶薄壁试样高温性能的重要因素,特别是通气状态的存在显著提高了其高温力学性能.      

喷嘴匹配方案及火焰筒开孔对燃烧室性能影响的试验研究

基于航空发动机主燃烧室扇形试验,针对点火喷嘴特性以及火焰筒大孔射流的改变对主燃烧室性能的改善情况进行了研究。试验中进行了点火用喷嘴匹配方案对燃烧室熄火性能,以及火焰筒大孔面积变化对燃烧室贫油熄火、燃烧效率和出口温度场性能影响的研究。研究结果表明：在供油系统设计中采用放大型点火喷嘴可改善主燃烧室贫油熄火性能;增大火焰筒主燃孔的面积可提高燃烧室的燃烧效率,改善出口温度场分布,而贫油熄火特性将变差;增大掺混孔的面积可提高燃烧室的燃烧效率,改善出口温度场分布,拓宽燃烧室的熄火动界．     

接受孔形状对预旋供气系统内气流流动影响研究

为对比不同形状接受孔的预旋系统内气流流动特性,通过数值模拟方法,对带有不同形状接受孔的预旋系统进行了研究。研究发现:收缩型接受孔入口截面气流流通面积较大,相对速度较小,在预旋系统中的性能最优,其次是类梯型,最后是直孔型。同一旋转雷诺数下,带收缩型接受孔的预旋系统无量纲温降较直孔型提高5.8%,总压损失系数降低3.0%。三种类型接受孔的预旋系统无量纲温降和总压损失系数均随进出口压比的增加而增大,在相同压比下,收缩型接受孔预旋系统无量纲温降最大,总压损失系数最小。     

含通孔损伤变截面钛合金蜂窝壁板拉伸性能研究

针对飞行器结构采用的钛合金蜂窝壁板,采用试验研究和有限元分析相结合的方法,研究了通孔损伤对变截面钛合金蜂窝壁板拉伸性能的影响.其中,有限元模型采用参数化建模方法建立,包含蜂窝芯体细节和斜角区细节结构.研究结果显示,斜角区是变截面钛合金蜂窝壁板的薄弱部位,无损伤试验件的破坏模式为沿斜角起始区域内蒙皮倒圆处横截面断裂;对于...     

开孔变刚度层合板压缩屈曲性能研究

针对开孔变刚度层合板,建立3种尺寸的层合板有限元模型,采用了线性屈曲、引入残余热应力的线性屈曲和引入初始缺陷的非线性屈曲的3种分析方法,研究了开孔层合板在压缩条件下的屈曲行为,并通过自动铺丝制造层合板进行试验对比,对3种方法的合理性进行了分析。结果表明,引入残余热应力的线性屈曲分析方法与试验结果最吻合,两者仅相差0.63%。基于该方法,讨论开孔层合板残余热应力分布特点和应力水平,得出了开孔层合板的应力分布云图和应力分布规律,计算出残余热应力对开孔复合材料层合的屈曲影响。结果表明,残余热应力对传统直线开孔层合板的屈曲载荷影响很小,仅提高了3.57%,但大大提高了变刚度开孔层合板的屈曲载荷,最多可达23.40%。说明纤维曲线铺放可以改变内部残余热应力的分布,提高整个开孔层合板承载压缩载荷的能力。     

硅微陀螺平板结构的压膜阻尼研究

压膜阻尼对硅微陀螺的精度具有重要影响。平板结构是硅微陀螺中一种典型结构,本文通过对雷诺方程的推导,得出平板在正弦规律小振幅刚性运动时的阻尼力解析式,并给出低频时阻尼系数的近似算法。利用Matlab和CoventorWare软件对运动平板的阻尼进行仿真计算,得出运动平板的阻尼系数和刚度系数,并分析平板参数对阻尼系数及刚度系数的影响。建立不同类型的带孔平板模型,通过比较可以看出,当阻尼孔按一定方式排列时,可以降低结构的阻尼。     

激光加工气膜孔对定向凝固高温合金薄壁持久性能的影响

采用定向凝固无余量精铸工艺制造的接近于空心涡轮叶片形状和壁厚的管状薄壁（δ＝１．２ｍｍ）试样,研究了激光加工孔对定向凝固高温合金薄壁持久性能的影响。结果表明,在９００℃／３７０ＭＰａ下,与没有孔的薄壁试样相比,有一排孔的试样持久性能没有明显降低,有两排孔的试样持久寿命略有下降。显微分析表明,激光加工孔对组织没有明显的影响,只是稍微减小了承载面积,而且只有在出现两排激光孔时才有所表现。     

Broadening of Fe X (6374 Å) profiles above the limb in a coronal hole

Profiles of the visible Fe X (6374 Å) coronal emission line as a function of height above the limb were obtained out to 1.16 solar radii in a coronal hole using the NSO/Sacramento Peak Observatory Coronagraph, Universal Spectrograph and a CCD camera. These are the first coronal line profiles obtained as a function of height in a coronal hole from the ground. Analysis of the line widths suggests a large component of nonthermal broadening which increases with height ranging from 40 to 60 km/s, depending upon the assumed temperature or thermal component of the profile.