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401.
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Lazarus A. J. Belcher J. W. Paularena K. I. Richardson J. D. 《Space Science Reviews》1998,83(1-2):87-92
We discuss the solar wind parameters measured in the distant heliosphere from the Voyager 2 spacecraft. Periodic variations in the speed of the wind observed at roughly the solar rotation period may correspond to interaction regions between slower and faster streams of wind. Since the interplanetary magnetic field is enhanced in such regions, they are important for the study of modulation of cosmic rays. Unfortunately, direct observation of the enhanced magnetic field from Voyager 2 has been made difficult by spacecraft-associated noise since 1989. 相似文献
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Klumpar D.M. Möbius E. Kistler L.M. Popecki M. Hertzberg E. Crocker K. Granoff M. Tang Li Carlson C.W. McFadden J. Klecker B. Eberl F. Künneth E. Kästle H. Ertl M. Peterson W.K. Shelly E.G. Hovestadt D. 《Space Science Reviews》2001,98(1-2):197-219
The Time-of-flight Energy Angle Mass Spectrograph (TEAMS) is being flown on the FAST Small Explorer mission to measure the 3-dimensional distribution function of the major ion species present in the lower magnetosphere. The instrument is similar to time-of-flight plasma analyzer systems that have been designed and planned for flight as CODIF (COmposition and DIstribution Function analyzer) on the four European Space Agency Cluster-II spacecraft and, as ESIC (Equator-S Ion Composition instrument) on Equator-S. This instrument allows the 3-dimensional distribution functions of individual ion species to be determined within
spin period (2.5 s). Two-dimensional distributions are measured in 80 ms. These capabilities are crucial for the study of selective energization processes in the auroral regions of the magnetosphere. The design, operational characteristics, and test and calibration results for this instrument are presented. The sensor consists of a toroidal top-hat electrostatic analyzer with instantaneous acceptance of ions over 360° in polar angle. After post-acceleration of the incoming ions by up to 25 kV, a time-of-flight mass spectrograph discriminates the individual species. It has been demonstrated through calibration that the instrument can easily separate H+, He2+, He+, O+ and, for energies after post-acceleration of > 20 keV, even O2
+ molecules. On-board mass discrimination and the internal accumulation of several distinct data quantities combined with the spacecraft's flexible telemetry formatting allow for instrument data rates from 7.8 kb s–1 to 315 kb s–1 to be telemetered to ground through the FAST centralized Instrument Data Processor. 相似文献
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Ergun R.E. Carlson C.W. Mozer F.S. Delory G.T. Temerin M. McFadden J.P. Pankow D. Abiad R. Harvey P. Wilkes R. Primbsch H. Elphic R. Strangeway R. Pfaff R. Cattell C.A. 《Space Science Reviews》2001,98(1-2):67-91
We describe the electric field sensors and electric and magnetic field signal processing on the FAST (Fast Auroral SnapshoT) satellite. The FAST satellite was designed to make high time resolution observations of particles and electromagnetic fields in the auroral zone to study small-scale plasma interactions in the auroral acceleration region. The DC and AC electric fields are measured with three-axis dipole antennas with 56 m, 8 m, and 5 m baselines. A three-axis flux-gate magnetometer measures the DC magnetic field and a three-axis search coil measures the AC magnetic field. A central signal processing system receives all signals from the electric and magnetic field sensors. Spectral coverage is from DC to 4 MHz. There are several types of processed data. Survey data are continuous over the auroral zone and have full-orbit coverage for fluxgate magnetometer data. Burst data include a few minutes of a selected region of the auroral zone at the highest time resolution. A subset of the burst data, high speed burst memory data, are waveform data at 2×106 sample s–1. Electric field and magnetic field data are primarily waveforms and power spectral density as a function of frequency and time. There are also various types of focused data processing, including cross-spectral analysis, fine-frequency plasma wave tracking, high-frequency polarity measurement, and wave-particle correlations. 相似文献
409.
贾德昌%周玉%雷廷权 《宇航材料工艺》2001,31(1):29-31
采用真空热压烧结工艺制备了SiO2短纤维补强增韧的SiO2玻璃陶瓷基复合材料,研究了烧结温度和保温时间对其显微结构和力学性能的影响规律,结果表明,SiO2f/SiO2复合材料的强度和韧性较石英玻璃有明显改善;延长热压保温时间、提高烧结温度、虽有利于材料致密化,但析晶量增加和纤维退化更严重,复合材料的强度和断裂韧性随之下降。 相似文献
410.
贾德昌%周玉%雷廷权%吴圣敏 《宇航材料工艺》2001,31(4):30-35
采用真空热压烧结工艺制备了碳纤维体积分数分别为20%、40%和60%的高致密Cf/SiO2复合材料,研究了碳纤维含量对其组织结构,力学性能、热膨胀特性和抗氧化性能的影响规律。结果表明:SiO2基体及20%Cf/SiO2复合材料中,SiO2仍保持非晶态,碳纤维含量为40%和60%时,SiO2发生部分析晶;Cf/SiO2复合材料的抗弯强度、断裂韧性和断裂应变,随碳纤维含量增加均呈现先降低后又增加的趋势,而弹性模量则先增后降;60%Cf/SiO2表现出明显伪塑性;碳纤维含量增大,使复合材料的热膨胀系数成倍增加,抗氧化性变差。 相似文献