卫星测量太阳耀斑对大气响应的一些目的和方法

S.V. Avakyan
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引用次数: 8

摘要

本文介绍了测量大气层对太阳耀斑反应的方法,包括小型系绳系统。小型系绳卫星非常适合于以下实验:高电离层光电子和俄歇电子能谱的测量,因为在大俯仰角没有来自卫星体的大阴影效应,而且来自卫星体的寄生光电子通量很小。2. 高层大气排放增加的测量和卫星辉光与其高度和尺寸之间关系的研究。3.测量电子和离子密度的增加,包括光学和质谱记录由于在无大气层高度的俄歇效应而形成的双带电荷的正离子。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Some purposes and methods of the satellite measurements of the ignorospheric response on the solar flares

The paper describes methods for measuring of the response of the ignorosphere to solar flares including small tethered systems. The small tethered satellites are very suitable for the following experiments: 1. Measurements of the high ionospheric photoelectron and Auger electron spectra because there is no large shadow effect from the satellite body at large pitch-angles and also parasitic photoelectron fluxes from the satellite body are small. 2. Measurements of the increase in emissions of the upper atmosphere and the investigation of the relationship between satellite glow and its altitude and dimensions. 3. Measurements of the increase in the electron and ion densities including optical and mass-spectrometric recording of the double charged positive ions which are formed due to Auger effect at the altitudes of ignorosphere.

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