2022
DOI: 10.1109/lawp.2022.3194693
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Modeling of Diurnal Variation Characteristics of VLF Wave Propagation in Earth-Ionosphere Waveguide With FDTD Method

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Cited by 4 publications
(6 citation statements)
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“…Very low frequency (VLF: 3–30 kHz) 1–5 has been widely applied in communication, 6 ionosphere detection, 7 as well as positioning, navigation, and timing systems 8 . Typical VLF ultra‐long‐range navigation systems, such as Omega and Alpha, provide global coverage, 9 whereas their cost of maintenance is very high.…”
Section: Introductionmentioning
confidence: 99%
“…Very low frequency (VLF: 3–30 kHz) 1–5 has been widely applied in communication, 6 ionosphere detection, 7 as well as positioning, navigation, and timing systems 8 . Typical VLF ultra‐long‐range navigation systems, such as Omega and Alpha, provide global coverage, 9 whereas their cost of maintenance is very high.…”
Section: Introductionmentioning
confidence: 99%
“…The numerical finite difference time domain (FDTD) [14][15][16][17][18][19][20][21][22][23] and finite-difference frequency domain (FDFD) 14 are common methods used to compute the VLF wave in the Earth-ionosphere waveguide. In 2017, Marshall et al 14 compared VLF signals simulated by the LWPC, FDTD, and FDFD models.…”
Section: Introductionmentioning
confidence: 99%
“…Direct measurements are difficult for large-scale efforts due to their high cost. Based on the exponential ionosphere profile [10][11][12][13][14][15] and International Reference Ionosphere (IRI) model, analytical and num erical methods are unable to accurately predict the VLF signal amplitude and phase in the waveguide. [24][25][26] Data for the time-and location-, instead of solar zenith angle-varying IRI electric density model may be insufficient or inaccurate for the lower ionosphere.…”
Section: Introductionmentioning
confidence: 99%
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