166 research outputs found
Photonic RF Channelization Based on Microcombs
In recent decades, microwave photonic channelization techniques have
developed significantly. Characterized by low loss, high versatility, large
instantaneous bandwidth, and immunity to electromagnetic interference,
microwave photonic channelization addresses the requirements of modern radar
and electronic warfare for receivers. Microresonator-based optical frequency
combs are promising devices for photonic channelized receivers, enabling full
advantage of multicarriers, large bandwidths, and accelerating the integration
process of microwave photonic channelized receivers. In this paper, we review
the research progress and trends in microwave photonic channelization, focusing
on schemes that utilize integrated microcombs. We discuss the potential of
microcomb-based RF channelization, as well as their challenges and limitations,
and provide perspectives for their future development in the context of on-chip
silicon-based photonics.Comment: This work has been submitted to the IEEE for possible publication.
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Circuits and architectures for the implementation of broadband channelizers
Broadband spectrum channelizers sub-divide a broadband input spectrum into multiple sub-bands, where each of the sub-bands is down-converted and further processed at baseband. These designs can help to relax baseband design specifications. For example, baseband analog-to-digital converters (ADCs) that process the sub-bands at the channelizer output see only a part of the incident spectrum. The sampling frequency, and potentially the dynamic range of each sub-band ADC can thus be relaxed, compared to the case where a single ADC is used to digitize the full spectrum.
Spectrum channelizers can be used for multiple applications. These designs can be used as general-purpose hybrid frequency-and-time domain ADCs. The designs can also be employed for spectrum analysis, as well as for wireless communication applications.
In this dissertation, two circuit techniques for the implementation of broadband channelizers are proposed. A frequency-translational feedback-based interference canceler for attenuating large interferers at the output of the front-end low-noise amplifier (LNA) of a channelizer is shown. The design uses harmonic rejection mixers (HRMs) with embedded frequency synthesis capability. While channelizers reduce the bandwidth and potentially the dynamic range of the baseband ADCs, the analog signal paths in the channelizer can be broadband. Consequently the dynamic range required of the analog section of a sub-band path can still be limited by the presence of large signals in other, potentially distant parts of the spectrum. The demonstrated design is useful for relaxing the dynamic range requirement of the analog section that follows the front-end LNA in a channelizer. Reduction of the harmonic response and the frequency synthesizer tuning-range is also achieved in this design.
Second, a two-stage HRM is proposed which shares the same bias current between the RF and baseband stages, thus reducing the power consumption. Issues arising from bias-current sharing, such as the 1/f noise of the RF stage and potential degradation of the 2nd harmonic response are identified, and circuit techniques are introduced to mitigate these potential degradation mechanisms.Electrical and Computer Engineerin
Utilizing tunable signal interference control topologies with electromechanical resonators
Exploiting knowledge gained from previous investigations of channelized and trans-versal filters, signal interference filters use transmission line differences to generate transmission zeros through phase-shifted combinations of signals at the output of a device. The transmission lines used in these circuits are straightforward to design, but are limited to high-frequency signals (on the order of a few gigahertz) due to the necessity for spatial compactness and low loss. More recent studies have used electromechanical resonators to achieve phase shifting and quality factor improvements at slightly-lower frequencies. These concepts may prove useful if extended to micro- and nanoscale resonators.
To explore signal interference topologies outside of purely-electrical, high-frequency filtering domains, a generic system model is proposed herein, which is based upon high quality factor resonant elements and continuously-tunable amplitude and phase components. The mathematical models developed in this work are generalized to apply the concept of signal interference to a variety of linear resonant systems. With this approach, frequency response behaviors can be quickly modified from amplification to cancellation through appropriate tuning of the phase and gain components.
The analytical models are simulated and implemented in electromechanical circuitry as a first step towards system integration. The prototypical circuits qualitatively match the desired frequency response and tuning behaviors, proving the use of the mathematical models in the design of linear resonant signal interference systems
A receiver with in-band IIP3>20dBm, exploiting cancelling of OpAmp finite-gain-induced distortion via negative conductance
Highly linear CMOS radio receivers increasingly exploit linear RF V-I conversion and passive down-mixing, followed by an OpAmp based Transimpedance Amplifier at baseband. Due to the finite OpAmp gain in wideband receivers operating with large signals, virtual ground is imperfect, inducing distortion currents. We propose to apply a negative conductance to cancel this distortion. In an RF receiver, this increases In-Band IIP3 from 9dBm to >20dBm, at the cost of 1.5dB extra NF and <10% power penalty. In 1MHz bandwidth, a Spurious-Free Dynamic Range of 85dB is achieved at <27mA up to 2GHz for 1.2V supply voltage
Advanced laser stratospheric monitoring systems analyses
This report describes the software support supplied by Systems and Applied Sciences Corporation for the study of Advanced Laser Stratospheric Monitoring Systems Analyses under contract No. NAS1-15806. This report discusses improvements to the Langley spectroscopic data base, development of LHS instrument control software and data analyses and validation software. The effect of diurnal variations on the retrieved concentrations of NO, NO2 and C L O from a space and balloon borne measurement platform are discussed along with the selection of optimum IF channels for sensing stratospheric species from space
Construction of FASR subsystem testbed and application for solar burst trajectories and RFI study
The construction of the Frequency Agile Solar Radiotelescope (FASR) Subsystem Testbed (FST) and observational results are described. Three antennas of Owens Valley Solar Array (OVSA) have been upgraded with newly designed, state of art technology. The 1-9 GHz RF signal from the antenna feed is transmitted via broadband (45 MHz-9.5 GHz) optical fiber links to the control room. The RF is then downconverted to a 500 MHz, single-sideband signal that can be tuned across the 1-9 GHz RF band. The data are sampled with an 8-bit, 1 GHz sampling-rate digitizer, and further saved to a computer hard disk. The full-resolution time-domain data thus recorded are then correlated through offline software to provide phase and amplitude spectra. An important feature of this approach is that the data can be reanalyzed multiple times with different digital signal-processing techniques (e.g., different bit-sampling, windowing, and RFI excision methods) to test the effects of different designs. As a prototype of the FASR system, FST provides the opportunity to study the design, calibration and interference-avoidance requirements of FASR. In addition, FST provides, for the first time, the ability to perform broadband spectroscopy of the Sun with high spectral, temporal and moderate spatial resolution. With this three-element interferometer, one has the ability to determine the location of simple sources with spectrograph-like time and frequency resolution.
The large solar flare of 2006 December 6 was detected by the newly constructed FASR Subsystem Testbed, which is operating on three antennas of Owens Valley Solar Array. This record-setting burst produced an especially fine set of fiber bursts--so-called intermediate-drift bursts that drift from high to low frequencies over 6-10 s. According to a leading theory (Kuijpers 1975), the fibers are generated by packets of whistler waves propagating along a magnetic loop, which coalesce with Langmuir waves to produce escaping electromagnetic radiation in the decimeter band. With this three element interferometer, for the first time fiber burst source locations can be determined relative to the background even though the absolute location is still unkown for the lack of phase calibration information. The radio information over a 500 MHz band (1.0-1.5 GHz) was used to determine the trajectories of the bursts.
Since the digital data are recorded with full resolution and processed offline, a key advantage of it is that one can process the data in different ways in order to simulate and test hardware implementations. FST data provides a unique testbed for studying methods of RFI excision. RFI is observed to be present in every one of the 500 MHz bands, and the high time and frequency resolution provided by FST allows one to characterize it in great detail. The use of time-domain kurtosis, and a variant of the kurtosis method in the frequency domain were explored to identify the presence of RFI and flag bad channels in simulated real time (i.e., we play back the raw, full-resolution recorded data and flag the bad channels during play-back just as a real-time system would do). The ability to select alternate RFI excision algorithms during play-back allows one to compare algorithms on an equal basis. From the same data set, the two kurtosis (time domain and frequency domain) RFI excision algorithms were compared. The results are compared quantitatively to show that the spectral kurtosis is more effective than time domain kurtosis algorithm for detecting the RFI contamination, as expected from theoretical considerations
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