Phenomena associated with complex (dusty) plasmas in the ionosphere during high-speed meteor showers

  • S. I. Kopnin
    RAS 1 Institute for Dynamics of Geospheres, , Moscow 119334, Russia
  • S. I. Popel
    RAS 1 Institute for Dynamics of Geospheres, , Moscow 119334, Russia
  • M. Y. Yu
    Zhejiang University 3 Department of Physics, Institute for Fusion Theory and Simulation, , Hangzhou 310027, China and Institute for Theoretical Physics I, , D-44780 Bochum, Germany

書誌事項

公開日
2009-06-01
DOI
  • 10.1063/1.3147931
公開者
AIP Publishing

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説明

<jats:p>Formation of dusty plasmas in the Earth’s ionosphere at 80–120 km altitudes during high-speed meteor showers and its detectable manifestations are discussed. Emphasis is given to ground-based observations such as detection of low-frequency (&lt;50 Hz) ionospheric radio noise, ground-based observations of infrasonic waves, and amplification of the intensity of green radiation at 557.7 nm from a layer at the 110–120 km altitude in the lower ionosphere. The physical processes responsible for these manifestations are considered.</jats:p>

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