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Fundamentals of Meteor Burst Communication
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Author(s): Ryoji Wakabayashi (Tokyo Metropolitan College of Industrial Technology, Japan)
Copyright: 2020
Pages: 11
Source title:
Analyzing the Physics of Radio Telescopes and Radio Astronomy
Source Author(s)/Editor(s): Kim Ho Yeap (Universiti Tunku Abdul Rahman, Malaysia)and Kazuhiro Hirasawa (University of Tsukuba, Japan)
DOI: 10.4018/978-1-7998-2381-0.ch011
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Abstract
When space dust rushes into the atmosphere, oxygen and nitrogen are ionized by frictional heat. Along the dust flight path, a very long cylindrical plasma tube, 10 meters in diameter and several kilometers long is formed. The long plasma tube is called “meteor burst” and is a good reflector for radio waves in the VHF band. Non-line-of-sight communication performed using this reflector is called “meteor burst communication”. In this chapter, the basics of meteor burst communication and its applications are outlined.
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