Mean energy of response to galactic cosmic ray spectrum: IMP 8 and Climax neutron monitor

Solar modulations of galactic cosmic ray (GCR) intensity contain a wealth of information about their transport in the heliosphere. To extract this information from the data one studies the dependence of the observed modulations on the mean energy of response of detectors providing data for the analyses. There is a great deal of confusion about the detector energy response to GCR spectrum in the literature. We present a preliminary report on the computations of the mean energy of response for the Climax neutron monitor (CL/NM) and IMP 8 cosmic ray nuclear composition instrument to GCR protons for 1973–1998, covering the solar cycles 21 and 22. We find that for penetrating proton channel on IMP 8 the mean energy changes by a factor of over two whereas for the neutron monitor the change is only 21%. However, the corresponding change for the computed modulation function is a factor of about 3.5.     

π-TFSK时频调制信号状态迁移的分析

本文主要对π－ＴＦＳＫ时频调制信号的状态迁移进行分析。首先，从数学模型出发，对π－ＴＦＳＫ时频调制信号的状态进行分析；然后，推出了该信号的状态迁移图；最后求出了π－ＴＦＳＫ时频调制信号的状态迁移矩阵。     

The Modulation of Galactic Cosmic Rays in the Heliosphere: Theory and Models

Almost all theoretical and numerical models for the modulation of cosmic ray in the heliosphere are based on Parker's transport equation which contains all the important basic physical processes. The relative importance of the various mechanisms is however not established and may vary significantly over 22 years. The simultaneous measurements of solar wind parameters, heliospheric magnetic field properties and cosmic rays over a wide range of energies and positions in the heliosphere have brought the realization that modulation is much more complicated than what the original drift models predicted. In the process the sophistication of models based on solving Parker's equation has increased by orders of magnitude. A short review of the global modulation of cosmic rays is given from a theoretical and modelling point of view.     

A calibration neutron monitor: Statistical accuracy and environmental sensitivity

This paper is a follow-on of that of Krüger et al. [Krüger, H., Moraal, H., Bieber, J.W., Clem, J.M., Evenson, P.A., Pyle, K.R., Duldig, M.L., Humble, J.E. A calibration neutron monitor: energy response and instrumental temperature sensitivity. J. Geophys. Res. 113, A08101, doi:10.1029/2008JA013229, 2008], that describes the characteristics of a pair of calibration neutron monitors that were developed to intercalibrate the count rates of the world’s neutron monitors against each other. Such an intercalibration will allow the calculation of energy (rigidity) spectra, which will enhance the quality of the neutron monitor data. Krüger et al. (2008) investigated the energy and temperature response of the calibrators. This paper studies the statistical accuracy of the calibration procedure, its repeatability, and the sensitivity to its environment. The paper concludes with a calibration procedure that can minimise the uncertainties caused by these five effects, or at least correct for them.     

某型飞机机身合拢总装型架设计新技术

某型飞机机身合拢总装型架，在设计上采用了先进制造技术。型架上装有目前国际先进的光学坐标系统，型架地基采用整体框架式底盘。型架结构为分散式。按飞机飞行状态在型架中摆放，并由上方起吊形式下架。本文简要介绍了该型架的设计、制造情况及效果。     

GaInP2外延膜中施主—受主对复合发光带的能量关量

通过变温与变激发强度的近红外光致发光研究了用ＭＯＣＶＤ方法、生长在ＧａＡｓ衬底上的Ｇａ０．５Ｉｎ０．５Ｐ（ＧａＩｎＰ２）外延薄膜的１．１７ｅＶ发射带的发光特性。１．１７ｅＶ发光带性质与０．９９ｅＶ及０．８５ｅＶ发光带的性质有着明显的差别。１．１７ｅＶ发光带的机理可用施主－受主对的复合发光来解释，其中施主－受主对系白处在Ｇａ格位上的Ｓｉ（ＳｉＧａ）及其最邻近的Ｇａ空位（ＶＧａ）所组成，记作ＳｉＧａ－ＶＧａ。考虑到ＧａＩｎＰ２中存在着很强的电子－格子耦合作用及其Ⅲ族子格子为部分有序，所以在施主－受主对复合发光中应计及Ｆｒａｎｃｋ－Ｃｏｎｄｏｎ位移△ＦＣ及该对在等效的部分有序势场中的相互作用能Ｅｓ（ＤＡＰ）。Ｘ—射线衍射实验表明，部分有序结构相当于成分调制，因而可用Ｋｒｏｎｉｇ－Ｐｅｎｎｅｙ模型来计算Ｅｓ（ＤＡＰ）值。这样，我们就导出了施主－受主对复合发光的新的能量表示式。     

微机在发展光学计测中的作用

通过列举材料，阐述了微型电子计算机的特点与功能，微机在光学计测中的作用，展望了微机在未来光学计测中的应用前景。     

π/4 D-QPSK基带调制解调的DSP实现

在以前的数字蜂窝系统中，往往采用FSK、ASK、PSK等调制方式。随着数字蜂窝系统的发展，对调制和数字蜂窝系统的技术要求也越来越高了。利用DSP手段，实现的π／4D—QPSK基带调制解调在技术要求方面要优于FSK、ASK、PSK等调制方式，更能满足数字蜂窝系统的要求。该技术的实现，提高了调制与解调的速度，为数字蜂窝系统的发展提供了更大的发展空间。     

基于STFRFT的LFM引信抗欺骗干扰方法

针对线性调频脉冲压缩引信易受转发式假目标欺骗干扰问题,提出了基于短时分数阶傅立叶变换(STFRFT)的抗欺骗干扰方法。首先,通过分数阶傅立叶变换将回波信号与欺骗干扰各分量信号进行分离;再利用相同调频率的LFM信号经短时分数阶傅立叶变换后最大幅值与窗函数宽度成线性关系,而不同调频率的最大幅值不随窗函数宽度变化的特点,有效分辨假目标欺骗干扰,正确检测目标回波信号;最后,通过仿真证明了方法的正确性,并验证所提方法具有良好的抗欺骗干扰效果。     

一种非接触光外差轮廓仪

介绍了一种纳米级非接触超高精度光外差轮廓仪。该量仪是基于普通光路的外差干涉仪,两束具有微小频差的激光束照射到制件表面:其中一束光被会聚后作为测量光针扫瞄制件表面;另一束光则被用作参考光束。这两束光经反射后形成干涉,所得信号的光程差与制件表面高度变化成正比。量仪的横向分辩力小于2μm,垂直分辩力小于1nm。制件不需要进行大的调整。制件表面同时亦被作为测量参考面。经光电转换后,信号由微机处理,从而快速完成测量、计算、显示与打印各种参数与图形。