270 likes | 445 Views
Some ionospheric effects on ground based radar. Y. Béniguel, J.-P. Adam. Total Electron Content (TEC) dependent effects (litterature review). Backscattering by electron density irregularities (litterature review). Scintillations (IEEA field of research). Ionospheric effects. Group delay
E N D
Some ionospheric effects on ground based radar Y. Béniguel, J.-P. Adam
Total Electron Content (TEC) dependent effects (litterature review). Backscattering by electron density irregularities (litterature review). Scintillations (IEEA field of research). Ionospheric effects
Group delay Dispersion Faraday rotation Direction of arrival TEC
Medium’s Characterisation Electron Density TEC map
Frequently at high latitude : Radar Auroral Clutter Possible impact : false targets Backscattering by electron density irregularities
Source : Stephen Quigley, “Space Weather System - Impact Products - SEEFS Overview” False targets
Temporal fluctuations of the trans-ionospheric signal : Amplitude Phase Polarization Direction of arrival Scintillations
POLAR CAP PATCHES AURORAL IRREGULARITIES SATCOM GPS PLASMA BUBBLES EQUATORIAL F LAYER ANOMALIES DAY NIGHT MAGNETIC EQUATOR SBR GPS SATCOM Geographical occurrence of scintillations
Scintillations Parameters S4 and sF S4 and are statistical variables computed over a “reasonable” time period that satisfies both good statistics and stationarity, as follows “Reasonable Time” depends primarily on the effective velocity of the Line of sight raypath; varies from 10 to 100 seconds; the phase is derived from detrended time series These quantities depend on the density fluctuations in the medium
GPS to monitor the Ionospheric Scintillations • GPS provides a convenient and cost effective way to monitor the ionospheric scintillations : many transmitting satellites + commercial receivers available. PRIS scintillation measurement campaign (ESTEC project) • S4 measured at GPS frequency (L-band) can be extrapolated to other frequencies : f-1.5 dependency
GISM to model the scintillations Phase Screen Technique target X The screen size is chosen in relation to the medium coherence length calculated by FFT radar
Amplitude (assuming an m-Nakagami distribution) : Rq : S4²=1/m for one way propagation Phase variance doubled Monostatic Radar : two ways effects
Medium’s Characterisation Fluctuations of the electron density S4 map / Phase map Mostly affects the equatorial regions -20° ML < < 20° ML
Effects on Radar Signal Processing Intensity scintillations C / N0 drops Phase scintillations increases the Doppler noise Angular and range errors increases the ambiguity Medium’s coherent time drops limit the integration time ( pb for low RCS targets)
Irregularities Spectrum & Intensity 3 parameters to define the spectrum : S4 = 0.25 5 dB ptp S4 = 0.53 13 dB ptp S4 = 0.66 20 dB ptp The slope p 2 < p < 5 The cut off frequency = f ( 1 / L0) The strength : usually 1 Hz value
Intensity Scintillations C / N0 drops of the fade depth level
Amplitude scintillation Power RCS fast fades Source : Knepp, « Altair VHF /UHF Observations of Multipath and Backscatter Enhancement », IEEE-AP, 1991
Angular Error (RMS) • The RMS angular error ( > 1° at 150 MHz) will increase the ambiguity and degrade the radar performances • The angular error is deduced from the phase autocorrelation function
Coherence Time • The coherence time limits the integration time and will degrade the radar performances for low RCS targets • The coherence time decreases when increasing S4
range spread range Doppler spread Doppler Doppler and range spreads • Phase fluctuations create Doppler spread • Multipath inside the medium create range spread
Doppler noise vs inhomogeneities average size Slope p = 3 L0 = 2500 m. L0 = 500 m.
Range delays due to scintillation ALTAIR Radar measurements at Kwajalein Island (4° North L) Source : D. Knepp IEEE-AP
Scattering function as compared to measurements Source : P. Cannon, N. Rogers, Qinetiq, Nottingham wkshp, Feb 2008
Conclusions • Ionosphere may limit significantly the radar performances especially for targets with low RCS • C / N0 may drop as much as 30 dB • The medium’s coherence time decreases when increasing scintillations (S4) and limit consequently the integration time • All the effects decrease roughly as f-1.5 but are very significant in the VHF and UHF frequency bands