Abstract

To provide theoretical guidance for the detection of ballistic missiles by skywave over-the-horizon radar, this paper first analyses the best way to detect ballistic missiles based on the rocket detection mechanism. Then using the diffusion model, chemical reaction model, and plasma diffusion model of neutral gas in the ionosphere, this paper studies the distribution of electrons and analyses the disturbance effect on the ionosphere caused by the release of ballistic missile exhaust plume in the ionosphere. Moreover, this paper considers the flight speed of the ballistic missile and the flow of the exhaust plume. Then the effects of different seasons, locations, and time zones on the release are compared. The results show that H2O can effectively dissipate background electrons to form spindle-shaped holes after release in the ionosphere. The height of the cavity radius corresponds to the peak of electron density of the background ionosphere, and the daytime dissipation is stronger than the nighttime dissipation, dissipation at low latitude is stronger than that at high latitude, and the seasonal difference is not obvious.

Highlights

  • When the Pioneer II was launched in 1959, Booker [1] first observed the existence of ionospheric holes using a drop tester and repeatedly observed the ionospheric holes generated by the rocket launch

  • Similar to the detection analysis based on plume, if the flight altitude satisfies the condition, the skywave radar can detect the ballistic missile based on the artificial ionospheric hole

  • According to the analysis of the mechanism of over-thehorizon radar in detecting rockets in the existing data, the feasibility of using an ionospheric hole formed by the plume to detect the ballistic missile is demonstrated

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Summary

Introduction

When the Pioneer II was launched in 1959, Booker [1] first observed the existence of ionospheric holes using a drop tester and repeatedly observed the ionospheric holes generated by the rocket launch. The principle and methods of detecting ballistic missile by over-the-horizon radar are roughly the same as those of detecting the launch vehicle; this includes the detection based on the missile itself, the plume, and the artificial ionosphere. The rocket is observed at approximately 100 km It is known from the previous analysis that skywave overthe-horizon radar can effectively detect the exhaust plume of the ballistic missile only in the ionosphere. This requires that the ballistic missile must fly higher than 60 km before the rocket shuts down. Similar to the detection analysis based on plume, if the flight altitude satisfies the condition, the skywave radar can detect the ballistic missile based on the artificial ionospheric hole. Compared with plume-based detection, artificial ionospheric holes are larger and wider, making it easier for skywave radar to detect targets

Model of the Artificial Ionospheric Hole Generated by Ballistic Missile
Numerical Simulation Results
Conclusion
Full Text
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