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951.
It is widely accepted that diffusive shock acceleration is an important process in the heliosphere, in particular in producing
the energetic particles associated with interplanetary shocks driven by coronal mass ejections. In its simplest formulation
shock acceleration is expected to accelerate ions with higher mass to charge ratios less efficiently than those with lower
mass to charge. Thus it is anticipated that the Fe/O ratio in shock-accelerated ion populations will decrease with increasing
energy above some energy. We examine the circumstances of five interplanetary shocks that have been reported to have associated
populations in which Fe/O increases with increasing energy. In each event, the situation is complex, with particle contributions
from other sources in addition to the shock. Furthermore, we show that the Fe/O ratio in shock-accelerated ions can decrease
even when the shock is traveling through an Fe-rich ambient ion population. Thus, although shock acceleration of an Fe-rich
suprathermal population has been proposed to explain large Fe-rich solar particle events, we find no support for this proposal
in these observations. 相似文献
952.
CMM曲线曲面测量领域的关键问题 总被引:11,自引:1,他引:10
分析了三坐标测量机曲线曲面测量领域涉及到的测量路径的生成、测球半径的补偿和曲线曲面数学模型的建立等几个关键问题和技术.阐述了CMM测量路径的生成方法和设计原则,分析了计算曲线曲面法失的常用方法以及给出了基于样条理论曲面拟合建模的一般数学模型. 相似文献
953.
根据国内飞机轮胎充气工作的现状,设计了一种基于放气控制的飞机轮胎自动充气装置,介绍了基于此种方式的充气及检测控制过程,针对以往充气装置的不足,此控制方式能够提高轮胎充气及检测的精度。并通过实验证明系统设计合理,满足设计要求,且系统效率高、性能稳定、操作方便,具有较好的经济效益及社会效益。 相似文献
954.
S. W. Kahler 《Space Science Reviews》2007,129(4):359-390
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. 相似文献
955.
数据采集器是飞行试验关键的测试设备,它的性能与现代飞机飞行试验有很大的关系.为满足现代飞机设计定型的需求,新一代数据采集器设计大量采用了FPGA和DSP器件,大大提高了采集器测量参数的采样率、通道数、测量参数类型和使用的灵活性.本文介绍的新一代采集器模拟量采集卡设计技术,用数字信号处理技术来实现信号的放大、滤波及偏置修正,并提供了对采集卡各个部分进行设计的理论依据. 相似文献
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