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At least 163 records · Page 9

A Compact Two-Stage 120 W GaN High Power Amplifier for SweepSAR Radar Systems

This work presents the design and measured results of a fully integrated switched power two-stage GaN HEMT high-power amplifier (HPA) achieving 60% power-added efficiency at over 120Woutput power. This high-efficiency GaN HEMT HPA is an enabling technology for L-band SweepSAR interferometric instruments that enable frequent repeat intervals and high-resolution imagery. The L-band HPA was designed using space-qualified state-of-the-art GaN HEMT technology. The amplifier exhibits over 34 dB of power gain at 51 dBm of output power across an 80 MHz bandwidth. The HPA is divided into two stages, an 8 W driver stage and 120 W output stage. The amplifier is designed for pulsed operation, with a high-speed DC drain switch operating at the pulsed-repetition interval and settles within 200 ns. In addition to the electrical design, a thermally optimized package was designed, that allows for direct thermal radiation to maintain low-junction temperatures for the GaN parts maximizing long-term reliability. Lastly, real radar waveforms are characterized and analysis of amplitude and phase stability over temperature demonstrate ultra-stable operation over temperature using integrated bias compensation circuitry allowing less than 0.2 dB amplitude variation and 2 deg phase variation over a 70 C range.

Thrivikraman, Tushar↗

High pulse rate high resolution optical radar system

The system is composed of an optical cavity with a laser and a mode locking means to build up an optical pulse. An optical switch is also provided within the cavity to convert the polarization of the optical pulse generated within the cavity. The optical switch comprises an electro-optical crystal driven by a time delayed driver circuit which is triggered by a coincident signal made from an optical pulse signal and a gating pulse signal. The converted optical pulse strikes a polarization sensitive prism and is deflected out of the cavity toward the pending target in the form of a pulse containing most of the optical energy generated by the laser in the pulse build-up period. After striking the target, the reflected energy is picked up by a transceiver with the total travel time of the pulse being recorded.

Goss, W. C.↗

Radar systems for the water resources mission, volume 3

Recent work was reviewed in the field of remote sensing relative to soil moisture. The target parameters were recognized that are necessary if optimum data retrieval is to be realized, and proper sensor instrumentation was recommended to achieve this goal.

Moore, R. K.↗

Ambiguities in spaceborne synthetic aperture radar systems

An examination of aspects of spaceborne SAR time delay and Doppler ambiguities has led to the formulation of an accurate method for the evaluation of the ratio of ambiguity intensities to that of the signal, which has been applied to the nominal SAR system on Seasat. After discussing the variation of this ratio as a function of orbital latitude and attitude control error, it is shown that the detailed range migration-azimuth phase history of an ambiguity is different from that of a signal, so that the images of ambiguities are dispersed. Seasat SAR dispersed images are presented, and their dispersions are eliminated through an adjustment of the processing parameters. A method is also presented which uses a set of multiple pulse repetition sequences to determine the Doppler centroid frequency absolute values for SARs with high carrier frequencies and poor attitude measurements.

Li, F. K.↗

Data reduction programs for a laser radar system

The listing and description of software routines which were used to analyze the analog data obtained from LIDAR - system are given. All routines are written in FORTRAN - IV on a HP - 1000/F minicomputer which serves as the heart of the data acquisition system for the LIDAR program. This particular system has 128 kilobytes of highspeed memory and is equipped with a Vector Instruction Set (VIS) firmware package, which is used in all the routines, to handle quick execution of different long loops. The system handles floating point arithmetic in hardware in order to enhance the speed of execution. This computer is a 2177 C/F series version of HP - 1000 RTE-IVB data acquisition computer system which is designed for real time data capture/analysis and disk/tape mass storage environment.

Badavi, F. F.↗

Saskatoon M. F. Radar System: (52 Deg N, 107 Deg W), Canada

The system runs continuously, producing 1-h profiles approx. 75 to 110 km, 1978 to 1983: in particular for the 30-d (Nov. 9 to Dec. 7), 10-d (Nov. 16 to 26), 4-d core periods (Nov. 19 to 23). The means (EW, NS) and fourier components (24-, 12-h) fitted for the 4-d are shown. s.d. are shown, as derived from four 24-h fits in the interval. Comparisons with the 10-, 30-d intervals confirm confidence in these data and the lack of major variability in November. The 1-h profiles are means of 12 profiles so intrinsic errors are minimal. The 4-, 10-d fourier fits are compared and also the 30-d means from 48-h fits; in these amplitudes are N2+E2 as N/E approx. 1. Means differ slightly due to planetary wave activity; 24-h tides are variable in Novembers; and the 12-h variation is small less than 80 km. The final figure is a high resolution spectra for the November month: the 12-, 24-h dominate; the 8-h appears less than 100 km; and up to 90 km there is a 4-d oscillation.

Manson, A. H.↗

May 1982, Saskatoon M. F. Radar System: (52 Deg N, 107 Deg W), Canada

The system runs continuously, producing 1-h profiles approx. 75 to 110 km, 1978 to 1983: in particular for the 30-d (April 20 to May 19) centered on the inner core (May 3 to 6), 10-d (May 2 to 11). Incredibly, the only days missed for April/May were May 4/5, so 4-d fits for the core could not made! However the winds and tides were stable during May, so that the 10-d fits can be taken for comparison with other locations. The means (EW/NS) and Fourier components (24-, 12-h) for the 10-d (May 2 to 11) are shown; also those for the 30 days. Standard deviations are shown to be quite small. There is also little difference between 10- and 30-d profiles. The zonal flow is quite weak, showing that the summer westward flow has not fully developed. The 24-h tide has large lambda: approx. 100 km (EW and infinity (NS). Below 90 km the tide is circular, but above almost linear with EW amplitudes larger than NS. The 12-h tide is circular and lambda is small below 95 km; and more linear and variable above. The 30-d May spectral figure shows that 12-, 24-h tides are comparable; otherwise there is a 3.85-d oscillation to approx. 90 km; there were no other significant peaks.

Manson, A. H.↗

Goldstone solar system radar

Information is provided about physical nature planetary surfaces and their topography as well as dynamical properties such as orbits and spin states using ground based radar as a remote sensing tool. Accessible targets are the terrestrial planets: the Earth's Moon, Mercury, Venus and Mars, the outer planets rings and major moons, and many transient objects such as asteroids and comets. Data acquisition utilizes the unique facilities of the Goldstone Deep Space Network, occasionally the Arecibo radar, and proposed use of the VLA (very large array).

Jurgens, R. F.↗

Goldstone solar system radar

Caltech/Jet Propulsion Laboratory (JPL) radar astronomers made use of the Very Large Array (VLA) at Socorro, NM, during February 1990, to receive radio echoes from the planet Venus. The transmitter was the 70 meter antenna at the Goldstone complex northwest of Barstow, CA. These observations contain new information about the roughness of Venus at cm to decimeter scales and are complementary to information being obtained by the Magellan spacecraft. Asteroid observations are also discussed.

Jurgens, Raymond F.↗

Wake Vortex Radar System Development: Overview

The objectives of the work are to: (1) Investigate microwave and millimeter wave sensors to locate, track, quantify, and observe the wake vortex hazard; (2) Develop and evaluate system concepts and designs using sensor system models and employing a theoretical reflectivity model for the wake vortex; (3) Test the validity of the theoretical model; (4) Acquire sensor systems and conduct field testing to evaluate; and to (5) Refine a system for field testing as a wake vortex sensor.

Neece, Robert T.↗