"资源一号"卫星星内高能粒子探测器

对空间辐射环境的效应以及“星内高能粒子探测器”原理和设计做了简要而全面地介绍，引用太阳活动宁静时期和一次剧烈的太阳扰动事件期间本仪器的观测数据显示了资料的质量和可用性。     

星内粒子辐射探测器上高压单元的模拟

中巴资源卫星上的星内粒子辐射探测器的探头必须要工作在稳定,高信噪比的直流高压电源下。事实证明,安装在中巴资源－1和中巴资源－2卫星上的探测器高压单元能够保证整个探测器的正常运行。但是,新的实验对高压单元的设计提出了新的要求和新的技术指标,作者根据要求和技术指标对原来的探测器高压单元部分进行了改进。首先简要介绍粒子辐射探测器以及它在空间探测方面的作用,然后介绍探测器高压单元的基本原理,并对其中的振荡－换能部分进行理论分析和数值模拟。通过数值模拟,可以从理论上预言高压单元工作点的稳定性以及输出电压随其他参数波动式的变化。最后,对所做的模拟进行相关的讨论和展望。     

Thermal experiment of silicon PIN detector

The experiment of this paper is the thermal test of the leakage current of silicon PIN detector. Raising temperature may cause the detector to increase leakage current, decrease depletion and increase noise. Three samples are used in the experiment. One (called ΔE) is the sample of 100 μm in thickness. The other two (called E₁ and E₂) are stacks of five detectors of 1000 μm in thickness. All of them are 12 mm in diameter. The experiment has been done for 21 hours and with power on continuously. The samples have undergone more than 60℃ for about one hour. They are not degenerated when back to the room temperature. The depletion rate is temperature and bias voltage related. With the circuit of the experiment and temperature at 35℃, ΔE is still depleted while E₁ and E₂ are 94.9% and 99.7% depleted respectively. The noises of the samples can be derived from the values at room temperature and the thermal dependence of the leakage currents. With the addition of the noise of the pre-amplifier, the noises of E₁, E₂ and ΔE at 24℃ are 16.4, 16.3, and 10.5 keV (FWHM) respectively while at 35℃ are about 33.6, 33.1, and 20.6 keV (FWHM) respectively.     

一种短波段电离层突然骚扰的连续监测设备

太阳耀斑爆发时将引起地球电离层的一系列突然扰动现象,称做电离层突然骚扰,即所谓的SID事件。由于这现事件严重地影响无线电通讯,同时,太阳耀斑爆发本身的机制也是太阳物理及日地物理中很重要的课题,需要对这些现象的形态学方面进行深入研究。因此,对耀斑及其伴随的各种现象的观测,记录监视及资料分析无论对国民经济以及基础天文和地球物理的研究都有着十分重要的意义。