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전리층 정밀 구조와 전자 포획

D층(60~90km): 낮에만 존재. E층(90~150km): 스포라딕E. F층(150~1000km): F1·F2로 분리, 전자 밀도 최고. 태양풍의 자유전자는 F층에서 가장 많이 포획된다.

📋 목차 6개 📖 APA 출처 7편
📚 참고문헌 APA 7판 (7편)
  • 1 Kelley, M. C. (2009). The Earth's ionosphere: Plasma physics and electrodynamics (2nd ed.). Academic Press.
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  • 4 Pobachenko, S. V., Kolesnik, A. G., Borodin, A. S., & Kalyuzhin, V. V. (2006). The contingency of parameters of human encephalograms and Schumann resonance electromagnetic fields. Biophysics, 51(3), 525–529.
  • 5 Cherry, N. J. (2002). Schumann resonances, a plausible biophysical mechanism. Natural Hazards, 26(3), 279–331.
  • 6 Volland, H. (Ed.). (1995). Handbook of atmospheric electrodynamics (Vol. 1). CRC Press.
  • 7 Price, C., Yair, Y., & Asfur, M. (2007). East Africa as the source of Schumann resonance background. Geophysical Research Letters, 34(4), L04103.