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101.
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
102.
The current status of the theory of a new astrophysical phenomenon, aradiation-driven diskon, is outlined.The cyclotron radiation pressure around sufficiently hot, strongly magnetized white dwarfs and neutron stars is shown to be able to drive a wind from the photosphere and support a plasma envelope in the closed part of the magnetosphere. The magnetohydrostatic configuration of an optically thin, radiatively supported plasma envelope is determined. It consists of an equatorial disk in the region where the cyclotron radiation force exceeds the local force of gravity and a closed shell near the equilibrium surface where the radiation pressure equals gravity. The effects of finite optical depth on the behaviour of the magnetospheric plasma and the influence of the envelope on the observed radiation are discussed.Classes of magnetic degenerate stars are pointed out in which radiation-driven diskons may be found. The best candidates are two individual stars, the strongly magnetized white dwarfs GD 229 and PG 1031+234. Both exhibit broad and deep depressions in the ultraviolet which are explained as a result of cyclotron scattering by an optically thick radiation-driven envelope in the inhomogeneous magnetic field of the star. We predict a temporal and spectral variability of these features due to non-stationary plasma motions in the envelope. 相似文献
103.
采用国产含氟乳液为基料,研究了辅料的种类和用量,涂料的组成及工艺参数对涂膜性能的影响,提出了能获得良好涂膜的NH-93型氟涂料的配方和成膜条件。 相似文献
104.
本文通过团体粉末渗铌试验,分析了渗剂成分、渗入时间与温度对不同材料渗层的影响,研究与探讨了渗层的组织和性能。对45钢、T10钢、9CrSi钢和GCr15钢等材料采用铌铁粉末进行的渗铌处理,均可形成一定厚度的铌渗层,且表层硬度提高很多,摩擦力矩数值反映渗铌后摩擦系数减少。 相似文献
105.
Observations carried out from the coronagraphs on board space missions (LASCO/SOHO, Solar Maximum and Skylab) and ground-based facilities (HAO/Mauna Loa Observatory) show that coronal mass ejections
(CMEs) can be classified into two classes based on their kinematics evolution. These two classes of CMEs are so-called fast
and slow CMEs. The fast CME starts with a high initial speed that remains more or less constant; it is also called the constant-speed CME. On the other hand, the slow CME starts with a low initial speed, but shows a gradual acceleration; it is also called
the accelerated and slow CME. Low and Zhang [Astrophys. J. 564, L53–L56, 2002] suggested that these two classes of CMEs could be a result of a difference in the initial topology of the
magnetic fields associated with the underlying quiescent prominences. A normal prominence magnetic field topology will lead
to a fast CME, while an inverse quiescent prominence results in a slow CME, because of the nature of the magnetic reconnection
processes. In a recent study given by Wu et al. [Solar Phys. 225, 157–175, 2004], it was shown that an inverse quiescent prominence magnetic topology also could produce a fast CME. In this
study, we perform a numerical MHD simulation for CMEs occurring in both normal and inverse quiescent prominence magnetic topology.
This study demonstrates three major physical processes responsible for destabilization of these two types of prominence magnetic
field topologies that can launch CMEs. These three initiation processes are identical to those used by Wu et al. [Solar Phys. 225, 157–175, 2004]. The simulations show that both fast and slow CMEs can be initiated from these two different types of magnetic
topologies. However, the normal quiescent prominence magnetic topology does show the possibility for launching a reconnection island (or secondary O-line) that might be thought of as a “CME’’. 相似文献
106.
如何实现学生从中学物理到大学物理学习的转变 总被引:2,自引:0,他引:2
贾君茹 《西安航空技术高等专科学校学报》2003,21(3):51-53
实现学生从中学物理学习到大学物理学习转变的关键是借助高等数学所揭示的数学方法的思想内涵 ,建立起从中学物理的不变到大学物理中变、从宏观到微观、从近似到精确这样一种贯穿于物理学始终的辩证唯物主义物理观。 相似文献
107.
T. Muoz-Darias I.G. Martínez-Pais J. Casares T.R. Marsh R. Cornelisse D. Steeghs V.S. Dhillon P.A. Charles 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2762-2764
We present preliminary results of a simultaneous X-ray/optical campaign of the prototypical LMXB Sco X-1 at 1–10 Hz time resolution. Lightcurves of the high excitation Bowen/HeII emission lines and a red continuum at λc 6000 Å were obtained through narrow interference filters with ULTRACAM, and these were cross-correlated with simultaneous RXTE X-ray lightcurves. We find evidence for correlated variability, in particular when Sco X-1 enters the Flaring branch. The Bowen/HeII lightcurves lag the X-ray lightcurves with a light travel time which is consistent with reprocessing in the companion star while the continuum lightcurves have shorter delays consistent with reprocessing in the accretion disc. 相似文献
108.
周兴生 《西安航空技术高等专科学校学报》2005,23(2):16-19
上世纪90年代以来,“传销”的蔓延造成了日益严重的社会问题。它源于行政法理论界探讨所得的“谨慎尝试”观对许可“传销”的倡言,但对这些法律研究的反思未曾开展。补作这项工作需要以系统法律理论分析“传销”及其相关问题。对德国新的《反不正当竞争法》第16条的系统分析显示,以普通法规制“传销”比以行政法有根本性优点。笔者进言采纳德国新的规制模式,以竞争法摧毁“传销”这种社会“顽疾”。 相似文献
109.
高职高专院校建设数字化校园过程中应注意的问题 总被引:1,自引:0,他引:1
21世纪以来,数字化和信息化成为现代社会的主要标志。高职高专院校为了提高自己的管理水平,跟上时代的步伐,也都在着手数字化校园的建设。本文从数字化校园的基本概念入手,介绍数字化校园的组成、建设内容、建设步骤以及建设过程中应注意的问题,并给出了数字化校园的基本模型。 相似文献
110.
用凝固模拟方法预测铝合金铸件缩松的形成 总被引:1,自引:0,他引:1
用有限元法和六节点等参数单元对铝合金金属型铸造过程进行了温度场的数值模拟,对铸件不同典型部位进行了金相分析,结果表明,参数G/可有效地预测铝合金缩松形成倾向的大小,计算值与实测值基本一致。 相似文献