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911.
912.
John Vallerga 《Space Science Reviews》1996,78(1-2):277-288
Because of the strong absorption of extreme ultraviolet radiation by hydrogen and helium, almost every observation with the Extreme Ultraviolet Explorer (EUVE) satellite is affected by the diffuse clouds of neutral gas in the local interstellar medium (LISM). This paper reviews some of the highlights of the EUVE results on the distribution and physical state of the LISM and the implications of these results with respect to the interface of the LISM and the heliosphere. The distribution of sources found with the EUVE all-sky surveys shows an enhancement in absorption toward the galactic center. Individual spectra toward nearby continuum sources provide evidence of a greater ionization of helium than hydrogen in the Local Cloud with an mean ratio of H I/He I of 14.7. The spectral distribution of the EUV stellar radiation field has been measured, which provides a lower limit to local H II and He II densities, but this radiation field alone cannot explain the local helium ionization. A combination of EUVE measurements of H I, He I, and He II columns plus the measurement of the local He I density with interplanetary probes can place constraints on the local values of the H I density outside the heliosphere to lie between 0.15 and 0.34 cm–3 while the H II density ranges between 0.0 and 0.14 cm–3. The thermal pressure (P/k = nT) of the Local Cloud is derived to be between 1700 and 2300 cm–3 K, a factor of 2 to 3 above previous estimates. 相似文献
913.
张为公 《南京航空航天大学学报》1993,25(5):700-705
本文就应变片直接测量应力的方法进行了探讨,提出二向应力片及三向应力片原理,使在实验应力分析的电测场合中,对于某点的应力分量的测量,无需进行几个应变片数据的分别采集,再综合成应力分量(正应力或剪应力),使读数应变与应力分量一一对应,且各测量数据之间在算法上没有耦合。二向应力片及三向应力片的使用,简化了测量数据的处理过程,在动态测量特别是冲击力测量中,具有一定的实用意义。 相似文献
914.
三相变压的联结组标号对其正常运行极为重要,必须校定,而目前变还缺少全面快捷的校定方法和设备。本文介绍采用微机系统来实现联结组桔的校定,首先把四类联结组差别区分开,然后分析指出同一类联结组中,除有六种正序标号外,存在六种逆序标号,提出用新的筛选法能简捷地判别校定同一类的十二种标号,当微机系统进行实际测试时,必须考虑电源电压三相不对称程序的影响,故经数学推导得出用实测计算值代替理想计算值作判别比较的基 相似文献
915.
在直11型机的适航审定时,按CCAR25.15(二)的要求,要进行功能-可靠性飞行试验,以验证该机是否满足CCAR27.1301(d)和CCAR27.1309(a)的要求。本文基于直11型机外场收集的可靠性信息,论述了该机的功能-可靠性与条例要求的相符性,从而把CCAR21所要求的功能-可靠性飞行验证时间减少为38小时,显然,这将减少飞行试验时间,加快试验进度,为今后用可靠性信息来验证新研直升机的功能-可靠性与适航条例要求相符性提供了合适的方法。 相似文献
916.
Alain Abergel Laurent Verstraete Christine Joblin René Laureijs Marc-Antoine Miville-Deschênes 《Space Science Reviews》2005,119(1-4):247-271
Infrared spectroscopy and photometry with ISO covering most of the emission range of the interstellar medium has led to important
progress in the understanding of the physics and chemistry of the gas, the nature and evolution of the dust grains and also
the coupling between the gas and the grains. We review here the ISO results on the cool and low-excitation regions of the
interstellar medium, where T
gas≲ 500 K, n
H∼ 100–105 cm−3 and the electron density is a few 10−4.
JEL codes: D24, L60, 047
Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries:
France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA. 相似文献
917.
Roger A. Kopp 《Space Science Reviews》1994,70(1-2):309-316
The working group on coronal streamers convened on the first day of the 2nd SOHO Workshop, which took place in Marciana Marina, Isola d'Elba, 27 September –1 October 1993. Recent progress in streamer observational techniques and theoretical modeling was reported. The contribution of streamers to the mass and energy supply for the solar wind was discussed. Moreover, the importance of thin electric current sheets for determining both the gross dynamical properties of streamers and the fine-scale filamentary structure within streamers, was strongly emphasized. Potential advances to our understanding of these areas of coronal physics that could be made by the contingent of instruments aboard SOHO were pointed out. 相似文献
918.
阐述了分布式计算机系统的基本原理以及互连方式,对其功能、特点进行了分析.为使该系统在民航等系统中的应用和研究更加广泛,文中还给出了一些应用实例. 相似文献
919.
王作光 《航空精密制造技术》1993,(2)
介绍采用霍尔开关测量角度系统动态精度的一种方法,详细介绍了动态检测装置、霍尔开关电路及其使用,最后对检测结果进行了分析讨论。 相似文献
920.
Cecile Gry 《Space Science Reviews》1996,78(1-2):239-246
The distribution, kinematics and physical properties of the interstellar matter surrounding the Sun can be inferred from ground-based and UV spectroscopic observations. On a 200 pc scale the local interstellar matter appears inhomogeneous and asymmetric. Although it generally flows towards the lower density region, it is composed of numerous small components a few parsecs in size with slightly different velocities. On a smaller scale the extent and the nature of the Local Cloud which flows over the Sun are discussed based on HST-GHRS observations of nearby stars. 相似文献