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71.
It is generally accepted that the energy that drives coronal mass ejections (CMEs) is magnetic in origin. Sheared and twisted
coronal fields can store free magnetic energy which ultimately is released in the CME. We explore the possibility of the specific
magnetic configuration of a magnetic flux rope of field lines that twist about an axial field line. The flux rope model predicts
coronal observables, including heating along forward or inverse S-shaped, or sigmoid, topological surfaces. Therefore, studying
the observed evolution of such sigmoids prior to, during, and after the CME gives us crucial insight into the physics of coronal
storage and release of magnetic energy. In particular, we consider (1) soft-X-ray sigmoids, both transient and persistent;
(2) The formation of a current sheet and cusp-shaped post-flare loops below the CME; (3) Reappearance of sigmoids after CMEs;
(4) Partially erupting filaments; (5) Magnetic cloud observations of filament material. 相似文献
72.
基于大规模定制的产品建模技术及配置过程研究 总被引:2,自引:0,他引:2
分析了三种主要的生产模式及其演变,在分析产品族结构形成过程的基础上提出基于配置单元的产品族结构模型,并对配置单元进行了论述。给出实现配置过程的算法并用实例进行验证。 相似文献
73.
We have obtained the first UV high resolution spectra of hot luminous stars in M31 with the FOS onHubble Space Telescope. The spectra, combined with optical spectroscopic and photometric observations, enable us to study their stellar winds and photospheric parameters. We derive mass-loss rates and velocity laws from the wind line profiles, with the SEI method, as well as information on abundances. The wind lines and photospheric spectra are compared with galactic stars of the same spectral type.The spectra analyzed so far indicate that the stars have mass-loss rates comparable or slightly lower than galactic stars of the same spectral type, but possibly different velocity laws in their winds. The spectra of two stars are discussed here. 相似文献
74.
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77.
针对大数据排序算法的需求,提出了基于任务驱动的并行排序算法。该算法采用任务驱动、AIO(Asynchronous Input/Output,异步输入/输出)和双缓冲区机制等技术充分利用系统资源;通过构造等价排序键,优化快速排序算法;并在算法实现上,采用多线程处理任务,通过控制线程个数控制并行度。综合利用这些技术,该算法使得大数据的排序性能接近理论极限值,在CPU(Central Processing Unit,中央处理器)资源充裕的情况下,利用异步压缩技术,还可以突破这一极限,最终实现的系统2 000s就可以对超过500Gbyte的磁盘数据做一次完整的排序。在数据库设计中充分利用此思想,将会实现连接和线程的分离,数据库将可以支持更大的连接数,从而提高数据库支持的并发度。 相似文献
78.
针对导航星座自主定轨中的星座整体旋转问题,采用增设少量地面锚固站的方法可有效解决该问题。通过推导星地距离对卫星轨道升交点赤经的偏导数,证明了星地距离对卫星轨道升交点赤经可观。仅考虑在我国大陆范围内布设锚固站的条件下,仿真分析了锚固站数量以及布局对导航星座自主定轨精度的影响。仿真实验结果表明:采用3个以上的锚固站,即可有效控制星座整体旋转,在14d的仿真时段内卫星自主定轨精度保持4m以内;锚固站数量越多,自主定轨精度越高,但随着锚固站数量的增加,自主定轨精度改善程度越来越小;在保持4个锚固站的情形下,采用不同的锚固站布局方案,自主定轨精度并无明显差别。 相似文献
79.
重量分布和重心位置是影响起落架和机体地面载荷的重要因素,其中商载是影响全机重心、惯量的最活跃因素。飞机实际运营中,有无穷多种商载分布及装载方案。为了确保机身载荷分析时,不遗漏严重设计情况,同时能大大减少载荷人员的工作量,本文对不同商载配置下的机身着陆载荷进行了研究分析,分析结果表明最大商载情况将构成机身垂直剪力和垂直弯矩的严重情况。因此,在进行机身载荷分析时,必须考虑最大商载情况,而最大燃油情况可以不必考虑。这一结论为今后有针对性的开展民机机身载荷分析提供了数据支持。 相似文献
80.
Understanding properties of solar energetic particle (SEP) events associated with coronal mass ejections has been identified
as a key problem in solar-terrestrial physics. Although recent CME shock acceleration models are highly promising, detailed
agreement between theoretical predictions and observations has remained elusive. Recent observations from ACE have shown substantial
enrichments in the abundances of 3He and He+ ions which are extremely rare in the thermal solar wind plasma. Consequently, these ions act as tracers of their source material,
i.e.,
3He ions are flare suprathermals and He+ ions are interstellar pickup ions. The average heavy ion composition also exhibits unsystematic differences when compared
with the solar wind values, but correlates significantly with the ambient suprathermal material abundances. Taken together
these results provide compelling evidence that CME-driven shocks draw their source material from the ubiquitous but largely
unexplored suprathermal tail rather than from the more abundant solar wind peak. However, the suprathermal energy regime has
many more contributors and exhibits much larger variability than the solar wind, and as such needs to be investigated more
thoroughly. Answers to fundamental new questions regarding the preferred injection of the suprathermal ions, the spatial and
temporal dependence of the various sources, and the causes of their variability and their effects on the SEP properties are
needed to improve agreement between the simulations and observations. 相似文献