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41.
D. J. Wu 《Space Science Reviews》2005,121(1-4):333-342
Nonthermal electrons play a major role during solar flares since not only they contain a large amount of the released energy
but also they provide important information of the flaring physics through their nonthermal radiation in radio and hard X-ray
bands. In a recent work Wu (Phys. Plasmas
10 (2003) 1364) proposed that dissipative solitary kinetic Alfvén wave (DSKAW) with a local shock-like structure could provide an efficient acceleration mechanism for energetic electrons in a
low-β plasma. In the present paper dynamical characteristics of the DSKAW acceleration mechanism in solar coronal plasmas
are studied and its application to the acceleration of flaring electrons is discussed. 相似文献
42.
日地共转扰动似稳结构及其反相现象在第21及22周再次显现,从而证实了上述发现是一种在长达世记的时间尺度内存在的普遍规律。包括1991-1992年内的百年地磁扰动资料还说明偶数太阳周的共转似稳结构扰动峰有逆太阳自转而线性性漂移的趋向。对即将来临的极小年前可能出现的共转扰动作了试验性的预测。 相似文献
43.
Shawqi Al Dallal 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
Diffuse Galactic gamma-ray flux resulting from the evaporation of primordial black holes has been the subject of intensive research work during the last few decades. Theoretical work addressing this issue started in the 1970s whereas data started pouring in only in the 1990s. We discuss in this paper a model of the potential contribution to the Galactic gamma-ray flux of primordial black holes in binary systems and extend the argument to include stable gravitational bound states called Holeums. The model has a predictive power and can be tested by looking for gamma-ray excess in the vicinity of violent events occurring in the Galaxy such as supernova explosions. 相似文献
44.
R. A. Leske R. A. Mewaldt C. M. S. Cohen A. C. Cummings E. C. Stone M. E. Wiedenbeck T. T. von Rosenvinge 《Space Science Reviews》2007,130(1-4):195-205
Solar energetic particles (SEPs) provide a sample of the Sun from which solar composition may be determined. Using high-resolution
measurements from the Solar Isotope Spectrometer (SIS) onboard NASA’s Advanced Composition Explorer (ACE) spacecraft, we have
studied the isotopic composition of SEPs at energies ≥20 MeV/nucleon in large SEP events. We present SEP isotope measurements
of C, O, Ne, Mg, Si, S, Ar, Ca, Fe, and Ni made in 49 large events from late 1997 to the present. The isotopic composition
is highly variable from one SEP event to another due to variations in seed particle composition or due to mass fractionation
that occurs during the acceleration and/or transport of these particles. We show that various isotopic and elemental enhancements
are correlated with each other, discuss the empirical corrections used to account for the compositional variability, and obtain
estimated solar isotopic abundances. We compare the solar values and their uncertainties inferred from SEPs with solar wind
and other solar system abundances and find generally good agreement. 相似文献
45.
We analyzed UVCS/SOHO data and compared the H I Lyα (121.6 nm) and O VI (103.2 nm, 103.7 nm) emission in the polar and equatorial
coronal holes. We found that the emission lines have similar characteristics in these two types of coronal holes. Both types
show evidence for superradially diverging boundaries. The latitudinal distribution of the O VI line ratio may indicate that
the equatorial coronal hole has O+5 outflow velocities lower than in the polar coronal holes.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
46.
R. M. Suleiman J.L. Kohl A. V. Panasyuk A. Ciaravella S.R. Cranmer L.D. Gardner R. Frazin R. Hauck P.L. Smith G. Noci 《Space Science Reviews》1999,87(1-2):327-330
The Ultraviolet Coronagraph Spectrometer (UVCS) on the Solar and Heliospheric Observatory (SOHO) has been used to measure
spectral line profiles for H I Lyα in the south polar coronal hole at projected heliocentric heights from 3.5 to 6.0 R⊙ during 1998 January 5–11. Observations from 1.5 to 2.5 R⊙ were made for comparison. The H I Lyα profile is the only one observable with UVCS above 3.5 R⊙ in coronal holes. Within this region the outflowing coronal plasma becomes nearly collisionless and the ionization balance
is believed to become frozen.
In this paper, the 1/e half widths of the coronal velocity distributions are provided for the observed heights. The velocity
distributions include all motions contributing to the velocities along the line of sight (LOS). The observations have been
corrected for instrumental effects and interplanetary H I Lyα. The half widths were found to increase with projected heliographic
height from 1.5 to 2.5 R⊙ and decrease with height from 3.5 to 5 R⊙.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
47.
<正> 一、前言 孔组位置度的计量,在没有专用量具的情况下,以通用量具计量的方法已有过不少讨论。而以计算机辅助计量的探讨,还是个新课题。本文利用计算机辅助数据处理,研究了6孔孔组位置度的计量方法。以孔位坐标、孔间距离及相邻两孔间的弧所对的中心角来建立判别式,作为计算机程序的数学模式,将各孔位坐标的计量数据键入计算机,即可得到结果。本文举例进行了验证。 相似文献
48.
复合材料结构广泛采用机械连接。由于孔轴配合中存在间隙,影响多孔连接的内力分配和接头强度。螺栓连接的过盈配合和铆钉连接都能消除间隙,但这样就造成孔轴相互挤压,因而引起应力,并可能造成局部损伤。本文探讨层板双孔过盈配合引起的应力,及讨论过盈配合应用的可能性。 相似文献
49.
G. M. Mason 《Space Science Reviews》2007,130(1-4):231-242
3He-rich solar energetic particle (SEP) events show huge enrichments of 3He and association with kilovolt electrons and Type-III radio bursts. Observations from a new generation of high resolution
instruments launched on the Wind, ACE, Yohkoh, SOHO, TRACE, and RHESSI spacecraft have revealed many new properties of these
events: the particle energy spectra are found to be either power-law or curved in shape, with the 3He spectrum often being distinctly different from other species. Ultra-heavy nuclei up to >200 amu are found to be routinely
present at average enrichments of >200 times solar-system abundances. The high ionization states previously observed near
∼1 MeV/nucleon have been found to decrease towards normal solar coronal values in these events. The source regions have been
identified for many events, and are associated with X-ray jets and EUV flares that are associated with magnetic reconnection
sites near active regions. This paper reviews the current experimental picture and theoretical models, with emphasis on the
new insights found in the last few years. 相似文献
50.
带孔复合材料层板动态拉伸破坏的应变率效应 总被引:1,自引:1,他引:0
采用三维Hashin准则作为纤维束损伤判据,根据材料不同损伤模式制定相应的材料性能退化方案,并考虑应变率效应对材料的强度性能进行修正,建立含孔复合材料层合板的渐进损伤分析模型,模拟材料在不同应变率下的损伤破坏过程。通过动态拉伸试验,获得材料在不同应变率下的载荷-位移关系及孔边不同位置的时间-应变关系,讨论了应变率对材料拉伸性能的影响及试件孔边的应力集中情况。有限元分析结果与试验数据相一致,证明了本文所提出分析模型的正确性和有效性。 相似文献