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The radar automatically tracks the strongest portion of the diffused echo, and, hence, the position coordinates measured by the radar correspond to the densest part of the diffused chaff cloud.
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Conventional pulse-echo ultrasonic techniques require sample dimensions large enough to avoid overlap of successive acoustic echoes and, hence, experimental volumes of several cubic millimeters, hardly compatible with experimentation at megabar pressures.
This is because the phase errors caused by the transmitter are the same in direct and echo pulses and hence can be counteracted; besides, as the direct and the echo pulses are received with small time difference, the phase errors caused by the receiver in direct and in echo pulses are nearly the same and also can be counteracted.
These sharp echoes appear as spikes in the overall time series of echo power and hence deletion of these points is necessary in order to obtain a correct result.
As an aside of the main objectives of the campaign, a dataset from a specially designed UAV flight around the radar was used to validate the Capon method for retrieving HR images of echo power and hence reinforce the capability of the radar to resolve fine-scale structures in the atmosphere, as shown in the section "Detection of UAVs by MU Radar".
This separation was made because metallic surgical clips are known to distort gradient echo images [ 27– 29] and hence were suspected to influence MRI-based quantification.
The enhancement of the low-level echo of the targets results in the increase of echo-to-clutter and noise ratio and hence better input for the target detectors.
From an acoustic point of view, the maximum magnitude is a modification of the echo reflection from the cartilage surface, and hence differences in the surface reflection indicate significant alterations in the acoustic impedance among degenerated cartilage samples.
Furthermore, early performance of focused echo allows for timely screening of sepsis-related myocardial dysfunction and hence more careful fluid administration and early inotropic support (vide infra).
(3) There exists no local time dependence and hence solar zenith angle dependence in the lifetime of mesospheric echoes which is confirmed from earlier rocket sonde data. .
There exists no local time dependence and hence solar zenith angle dependence in the lifetime of mesospheric echoes which is confirmed from earlier rocket sonde data.
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