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Theory and simulation of ionospheric effects on synthetic aperture radar

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Theory and simulation of ionospheric effects on synthetic aperture radar. / Belcher, David; Rogers, Neil.
In: IET Radar Sonar and Navigation, Vol. 3, No. 5, 10.2009, p. 541-551 .

Research output: Contribution to Journal/MagazineJournal articlepeer-review

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Belcher D, Rogers N. Theory and simulation of ionospheric effects on synthetic aperture radar. IET Radar Sonar and Navigation. 2009 Oct;3(5):541-551 . doi: 10.1049/iet-rsn.2008.0205

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Belcher, David ; Rogers, Neil. / Theory and simulation of ionospheric effects on synthetic aperture radar. In: IET Radar Sonar and Navigation. 2009 ; Vol. 3, No. 5. pp. 541-551 .

Bibtex

@article{955ee396428e41be9f10f86c5d6b3ac3,
title = "Theory and simulation of ionospheric effects on synthetic aperture radar",
abstract = "Space-based synthetic aperture radar (SAR) necessarily involves imaging through the ionosphere. At low frequencies (VHF, UHF and L-band) the ionosphere will degrade the SAR image. Previous work has shown that the amount of image degradation strongly depends on the integrated strength of ionospheric turbulence, C k L. The focusing, sidelobes and integrated sidelobe ratio all depend on C k L in a manner that can be directly predicted by a simple analytic theory, which is reviewed and extended to cover any synthetic aperture length. Simulations of the ionosphere, using a thin phase screen parabolic equation approach, are performed under different ionospheric conditions for a number of possible SAR systems and the results compared with the analytic theory. It is concluded that, provided that the scattering is weak, the theory represents a good predictor of SAR performance, even at UHF. The known statistics of C k L can therefore be used to predict the performance of any trans-ionospheric SAR without performing a simulation.",
author = "David Belcher and Neil Rogers",
year = "2009",
month = oct,
doi = "10.1049/iet-rsn.2008.0205",
language = "English",
volume = "3",
pages = "541--551 ",
journal = "IET Radar Sonar and Navigation",
issn = "1751-8784",
publisher = "Institution of Engineering and Technology",
number = "5",

}

RIS

TY - JOUR

T1 - Theory and simulation of ionospheric effects on synthetic aperture radar

AU - Belcher, David

AU - Rogers, Neil

PY - 2009/10

Y1 - 2009/10

N2 - Space-based synthetic aperture radar (SAR) necessarily involves imaging through the ionosphere. At low frequencies (VHF, UHF and L-band) the ionosphere will degrade the SAR image. Previous work has shown that the amount of image degradation strongly depends on the integrated strength of ionospheric turbulence, C k L. The focusing, sidelobes and integrated sidelobe ratio all depend on C k L in a manner that can be directly predicted by a simple analytic theory, which is reviewed and extended to cover any synthetic aperture length. Simulations of the ionosphere, using a thin phase screen parabolic equation approach, are performed under different ionospheric conditions for a number of possible SAR systems and the results compared with the analytic theory. It is concluded that, provided that the scattering is weak, the theory represents a good predictor of SAR performance, even at UHF. The known statistics of C k L can therefore be used to predict the performance of any trans-ionospheric SAR without performing a simulation.

AB - Space-based synthetic aperture radar (SAR) necessarily involves imaging through the ionosphere. At low frequencies (VHF, UHF and L-band) the ionosphere will degrade the SAR image. Previous work has shown that the amount of image degradation strongly depends on the integrated strength of ionospheric turbulence, C k L. The focusing, sidelobes and integrated sidelobe ratio all depend on C k L in a manner that can be directly predicted by a simple analytic theory, which is reviewed and extended to cover any synthetic aperture length. Simulations of the ionosphere, using a thin phase screen parabolic equation approach, are performed under different ionospheric conditions for a number of possible SAR systems and the results compared with the analytic theory. It is concluded that, provided that the scattering is weak, the theory represents a good predictor of SAR performance, even at UHF. The known statistics of C k L can therefore be used to predict the performance of any trans-ionospheric SAR without performing a simulation.

U2 - 10.1049/iet-rsn.2008.0205

DO - 10.1049/iet-rsn.2008.0205

M3 - Journal article

VL - 3

SP - 541

EP - 551

JO - IET Radar Sonar and Navigation

JF - IET Radar Sonar and Navigation

SN - 1751-8784

IS - 5

ER -