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<p>We present the results of measuring intensity variations of atmospheric emission in the 630, 557.7, and 391.4 nm lines, caused by the impact of high-power short-wave radio emission of the Sura heating facility on the ionosphere. The data were obtained using a three-channel photometer located in the immediate vicinity of the heater. In the experiments of 2023 and 2024, a regular increase in the emission intensity in the 391.4 and 557.7 nm lines, induced by the Sura radiation, was recorded for the first time.</p>

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Artificial Optical Luminescence of the Ionosphere in the 557.7 nm and 391.4 nm Lines Stimulated by Short-Wave Radio Emission from the Sura Facility

  • 期刊论文

  • 发表日期：

    2025年3月1日

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  • I. D. Tkachev,
  • A. B. Beletsky,
  • S. M. Grach,
  • I. A. Nasyrov,
  • A. V. Shindin,
  • D. A. Kogogin

摘要

We present the results of measuring intensity variations of atmospheric emission in the 630, 557.7, and 391.4 nm lines, caused by the impact of high-power short-wave radio emission of the Sura heating facility on the ionosphere. The data were obtained using a three-channel photometer located in the immediate vicinity of the heater. In the experiments of 2023 and 2024, a regular increase in the emission intensity in the 391.4 and 557.7 nm lines, induced by the Sura radiation, was recorded for the first time.