Standard

Wideband scattering functions for HF ionospheric propagation channels. / Gherm, Vadim E.; Zernov, Nikolay N.; Lundborg, Bengt; Darnell, Michael; Strangeways, Hal J.

в: Journal of Atmospheric and Solar-Terrestrial Physics, Том 63, № 14, 09.2001, стр. 1489-1497.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

Harvard

Gherm, VE, Zernov, NN, Lundborg, B, Darnell, M & Strangeways, HJ 2001, 'Wideband scattering functions for HF ionospheric propagation channels', Journal of Atmospheric and Solar-Terrestrial Physics, Том. 63, № 14, стр. 1489-1497. https://doi.org/10.1016/S1364-6826(01)00037-2

APA

Gherm, V. E., Zernov, N. N., Lundborg, B., Darnell, M., & Strangeways, H. J. (2001). Wideband scattering functions for HF ionospheric propagation channels. Journal of Atmospheric and Solar-Terrestrial Physics, 63(14), 1489-1497. https://doi.org/10.1016/S1364-6826(01)00037-2

Vancouver

Gherm VE, Zernov NN, Lundborg B, Darnell M, Strangeways HJ. Wideband scattering functions for HF ionospheric propagation channels. Journal of Atmospheric and Solar-Terrestrial Physics. 2001 Сент.;63(14):1489-1497. https://doi.org/10.1016/S1364-6826(01)00037-2

Author

Gherm, Vadim E. ; Zernov, Nikolay N. ; Lundborg, Bengt ; Darnell, Michael ; Strangeways, Hal J. / Wideband scattering functions for HF ionospheric propagation channels. в: Journal of Atmospheric and Solar-Terrestrial Physics. 2001 ; Том 63, № 14. стр. 1489-1497.

BibTeX

@article{f2fb6f36f55a41ebb089fcf72433ae6e,
title = "Wideband scattering functions for HF ionospheric propagation channels",
abstract = "A physically based method has been developed to simulate the wideband HF ionospheric propagation channel relevant to the case of wideband spread spectrum HF communications and also other HF applications such as digital broadcasting and over-the-horizon radar. It is based on the consideration and solution of the equations governing pulse signal propagation through a fluctuating time varying random ionosphere. The wideband scattering function has been constructed as the appropriate Fourier transform of the correlation function of a channel impulse response. Numerical codes have been written, which allow numerical simulation of the wideband scattering function of the HF sky wave ionospheric fluctuation channel for any given model of the background ionosphere and time varying ionospheric turbulence with an anisotropic inverse power law spatial spectrum and frozen drift of the ionospheric inhomogeneities. When employed in the simulation of the scattering function for real conditions of propagation, the method provides the possibility of analysing the propagation effects for different relative bandwidths of the background channel, fluctuating channel and transmitted pulse. The effects of the transmitted pulse bandwidth and anisotropy of the irregularities have been studied. The numerical results have been obtained and presented, which demonstrate the contribution of the effects enumerated in the wideband scattering function of the HF ionospheric channel.",
keywords = "Anisotropy, Fluctuating ionosphere, Scattering function, Sky wave ionospheric channel",
author = "Gherm, {Vadim E.} and Zernov, {Nikolay N.} and Bengt Lundborg and Michael Darnell and Strangeways, {Hal J.}",
note = "Publisher Copyright: {\textcopyright} 2001 Elsevier Science Ltd",
year = "2001",
month = sep,
doi = "10.1016/S1364-6826(01)00037-2",
language = "English",
volume = "63",
pages = "1489--1497",
journal = "Journal of Atmospheric and Solar-Terrestrial Physics",
issn = "1364-6826",
publisher = "Elsevier",
number = "14",

}

RIS

TY - JOUR

T1 - Wideband scattering functions for HF ionospheric propagation channels

AU - Gherm, Vadim E.

AU - Zernov, Nikolay N.

AU - Lundborg, Bengt

AU - Darnell, Michael

AU - Strangeways, Hal J.

N1 - Publisher Copyright: © 2001 Elsevier Science Ltd

PY - 2001/9

Y1 - 2001/9

N2 - A physically based method has been developed to simulate the wideband HF ionospheric propagation channel relevant to the case of wideband spread spectrum HF communications and also other HF applications such as digital broadcasting and over-the-horizon radar. It is based on the consideration and solution of the equations governing pulse signal propagation through a fluctuating time varying random ionosphere. The wideband scattering function has been constructed as the appropriate Fourier transform of the correlation function of a channel impulse response. Numerical codes have been written, which allow numerical simulation of the wideband scattering function of the HF sky wave ionospheric fluctuation channel for any given model of the background ionosphere and time varying ionospheric turbulence with an anisotropic inverse power law spatial spectrum and frozen drift of the ionospheric inhomogeneities. When employed in the simulation of the scattering function for real conditions of propagation, the method provides the possibility of analysing the propagation effects for different relative bandwidths of the background channel, fluctuating channel and transmitted pulse. The effects of the transmitted pulse bandwidth and anisotropy of the irregularities have been studied. The numerical results have been obtained and presented, which demonstrate the contribution of the effects enumerated in the wideband scattering function of the HF ionospheric channel.

AB - A physically based method has been developed to simulate the wideband HF ionospheric propagation channel relevant to the case of wideband spread spectrum HF communications and also other HF applications such as digital broadcasting and over-the-horizon radar. It is based on the consideration and solution of the equations governing pulse signal propagation through a fluctuating time varying random ionosphere. The wideband scattering function has been constructed as the appropriate Fourier transform of the correlation function of a channel impulse response. Numerical codes have been written, which allow numerical simulation of the wideband scattering function of the HF sky wave ionospheric fluctuation channel for any given model of the background ionosphere and time varying ionospheric turbulence with an anisotropic inverse power law spatial spectrum and frozen drift of the ionospheric inhomogeneities. When employed in the simulation of the scattering function for real conditions of propagation, the method provides the possibility of analysing the propagation effects for different relative bandwidths of the background channel, fluctuating channel and transmitted pulse. The effects of the transmitted pulse bandwidth and anisotropy of the irregularities have been studied. The numerical results have been obtained and presented, which demonstrate the contribution of the effects enumerated in the wideband scattering function of the HF ionospheric channel.

KW - Anisotropy

KW - Fluctuating ionosphere

KW - Scattering function

KW - Sky wave ionospheric channel

UR - http://www.scopus.com/inward/record.url?scp=2142842160&partnerID=8YFLogxK

U2 - 10.1016/S1364-6826(01)00037-2

DO - 10.1016/S1364-6826(01)00037-2

M3 - Article

AN - SCOPUS:2142842160

VL - 63

SP - 1489

EP - 1497

JO - Journal of Atmospheric and Solar-Terrestrial Physics

JF - Journal of Atmospheric and Solar-Terrestrial Physics

SN - 1364-6826

IS - 14

ER -

ID: 78885717