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The ionosphere as a focusing lens: A case study involving simultaneous type III solar radio storm measurements from the ISIS 1 and 2 and ISEE 3 satellites

机译:电离层作为聚焦透镜:一个案例研究,涉及同时测量ISIS 1和2和ISEE 3卫星的III型太阳射电风暴

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摘要

For several decades ionospheric focusing has been suggested as a means of improving antenna resolution at frequencies less than about 10 MHz for the observations of spatial features of the cosmic noise background as well as the spectra of discrete radio sources. In this paper the possibility of using terrestrial ionospheric focusing to improve the directivity of electric dipoles on space missions has been investigated by comparing simultaneous observations of a solar radio storm by the ISIS 1 and ISIS 2 spacecraft, in near Earth orbit, and the ISEE 3 spacecraft located beyond the magnetosphere. To this end, a three-dimensional ray tracing in a spherically stratified ionosphere has been carried out for conditions appropriate to the observations by the ISIS spacecraft of a solar radio storm in September 1983. This procedure allows Poynting flux spectral densities measured on ISIS to be converted to spectral densities well outside the ionosphere where they can be compared directly with simultaneous observations on ISEE 3. The results demonstrate good agreement over their common observing frequency range (1–2 MHz). Furthermore, since ISIS covers higher frequencies than ISEE 3, the spectrum of the solar radio storm was extended to 4 MHz.
机译:几十年来,已经提出了电离层聚焦作为提高天线分辨率的一种手段,该方法可以在小于约10 MHz的频率上观察宇宙噪声背景的空间特征以及离散无线电源的频谱。在本文中,通过比较ISIS 1和ISIS 2航天器在近地轨道以及ISEE 3上对太阳无线电风暴的同步观测,研究了使用电离层聚焦来改善太空任务中电偶极子指向性的可能性。位于磁层以外的航天器。为此,在1983年9月ISIS航天器对太阳射电暴的观测条件下,在球形分层电离层中进行了三维射线追踪。转换为电离层外的光谱密度,可以将它们直接与同时进行的ISEE 3观测进行比较。结果表明,在它们的共同观测频率范围(1-2 MHz)中,它们具有很好的一致性。此外,由于ISIS覆盖的频率高于ISEE 3,因此太阳无线电风暴的频谱扩展到了4 MHz。

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