Protecting the DSN from RFI from earth orbiters: experience, tools, development status and lessons learned
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RFI DSN interference↗
Engineering topics
Manshadi, F.
Publications and source records attributed to Manshadi, F..
Can MRO send 6 Mbps telemetry using x-band channel 32?
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MRO interference↗
Small omni-directional antenna development for Mars Sample Return Mission
This work addresses the design, analysis and test of omni-directional antennas at 401.5 MHz and 437.1 MHz frequencies, on Mars Orbital Sample (OS) return canisters, which are part of a Mars Sample Return (MSR) mission.
antennas sample return omni-directional small ante↗
The Ultra Low Noise Diplexed X-Band Microwave Feed for NASA 70-m Antennas
This paper describes the configuration, detail design, and performance of a new ultra low noise diplexed X-band microwave feed system, called X/X diplexing feed, for the Deep Space Network (DSN) 70-m antennas.
microwave feed diplexed antenna low noise X-band↗
Millimeter/Submillimeter Wave Communications Via Ceramic Ribbon
Finding very low loss waveguides in the millimeter/submillimeter wave range has been a problem of considerabel interest for many years. Starting from fundamentals, we have found a new way to design a waveguide structure which is capable of providing an attenuation coefficient of less than 10dB/km for the guided dominant mode.
Ceramic Ribbon millimeter wave waveguide wave rang↗
The S/X-Band Microwave Feed System for NASA's First Beamwaveguide Antenna
The configuration, detail design, and performance of a dual S/X- band microwave feed system for the first Deep Space Network beamwaveguide antenna is reported. This antenna, which is primarily used for research and development tasks, is an elevation-over-azimuth type using wheel and track azimuth bearings. The S/X-band microwave feed system is super low noise for support of deep space missions.
microwave↗
A Novel Design Technique for Beam-Waveguide Antennas
The new 34-m beam-waveguide (BWG) antenna at Goldstone has a beam magnifier ellipse below ground level that transforms a 22-dB gain feedhorn into a high-gain 29-dB gain pattern for input to a standard four-mirror BWG system. It was initially designed for the X- an Ka-bands, and has a loss of less than 0.2 dB.
antenna↗
The S/X-Band Microwave Feed System for NASA's First Beamwaveguide Antenna
The configuration, detail design, and performance of the dual S/X-band microwave feed system for the first Deep Space Network (DSN) beamwaveguide (BWG) antenna are reported int his paper. By using existing spare components, simplifying the design of new components, and using new fabrication techniques and material, this feed system was implemented successfully with a small budget and a very tight schedule. The measured noise temperature of the feed systems is 17.5 Kelvin for S-band and 24.0 Kelvin for X-band, which agrees very closely with the predicted performance.
S/X-Band↗
Novel solutions to low-frequency problems with geometrically designed beam-waveguide systems
The poor low-frequency performance of geometrically designed beam-waveguide (BWG) antennas is shown to be caused by the diffraction phase centers being far from the geometrical optics mirror focus, resulting in substantial spillover and defocusing loss. Two novel solutions are proposed: (1) reposition the mirrors to focus low frequencies and redesign the high frequencies to utilize the new mirror positions, and (2) redesign the input feed system to provide an optimum solution for the low frequency. A novel use of the conjugate phase-matching technique is utilized to design the optimum low-frequency feed system, and the new feed system has been implemented in the JPL research and development BWG as part of a dual S-/X-band (2.3 GHz/8.45 GHz) feed system. The new S-band feed system is shown to perform significantly better than the original geometrically designed system.
Imbriale, W. A.↗
DSS-13 S-/X-band microwave feed system
The configuration, detail design, and performance of the dual S-/X-band microwave feed system for the new DSN beam-waveguide antenna, Deep Space Station (DSS) 13, are reported. By using existing spare components, reducing fabrication cost of new components by simplifying their design, and using new fabrication techniques and material, this DSS-13 feed system was implemented successfully with a small budget and a very tight schedule. Measured noise temperature gains of the feed system are 17.5 K for S-band (2200-2300 MHz) and 24.0 K for X-band (8200-8600 MHz), which agree very closely with the predicted performance.
Manshadi, F.↗
Microwave feed systems for NASA's beam-waveguide reflector antennas
The major features of a beam waveguide (BWG) antenna and the variety of feed system configurations that can be used with this type of antenna are described. The first BWG antenna built by NASA (DSS 13), and its microwave feed systems and their major components, such as the low noise amplifiers, passive microwave components, and the frequency selective mirrors used for multiple frequency operation or diplexing purpose, are discussed.
Manshadi, F.↗
Earth-based antenna network tradeoffs for NASA's Space Exploration Initiative (SEI)
The results of a tradeoff study conducted for selection of the most viable earth-based antenna network architecture for support of NASA's Space Exploration Initiative (SEI) lunar and mars missions are summarized. The study addressed the lunar mission support requirements, and examined the performance, operations, and cost tradeoffs of using either the NASA Deep Space Network (DSN) large 34-m antennas or smaller commercial antennas to replace or supplement the 34-m antennas. The results are presented as a set of eight tables.
Manshadi, F.↗
End-loaded crossed-slot radiating elements
Three cavity-backed crossed-slot antenna configurations are described that offer simple design, easy frequency tuning, light weight, low loss, and low cost. These antennas are designed for mobile satellite (MSAT) vehicle phased-array applications. The slots in these antennas are end-loaded. The end loading makes the slots effectively longer, and hence reduces their resonant frequency. Therefore, relatively small radiating elements can be achieved for large-angle-scanning phased-array antennas. These antennas have good RF characteristics and provide a relatively wide bandwidth without needing external tuning circuits for impedance matching. Measurements for the return loss and the far-field pattern of these antennas are presented.
Manshadi, F.↗
Technology challenges and trade-offs in application of multiple-beam antennas to NASA's Personal Access Satellite System
A review is presented of the trade-offs and technology challenges that exist in developing the multiple-beam satellite antennas for NASA's Personal Access Satellite System. Different types of multiple-beam antenna systems that can provide full coverage of the CONUS such as switched beam, fixed beam, or scanned beam systems are examined. Some techniques for interbeam power management for efficient utilization of satellite power and reliable operation are discussed.
Manshadi, F.↗
Hypercube-Computer Analysis Of Electromagnetic Scattering
Capabilities of hypercube and parallel processing demonstrated. Report describes use of Mark III Hypercube computer to analyze scattering of electromagnetic waves. Purpose of study to assess utility of parallel computing in such computation-intensive problems as large-scale electromagnetic scattering. Two electromagnetic codes based on different algorithms converted to run on Mark III Hypercube. First code implements finite-difference, time-domain solution of Maxwell's curl equations. Second code is Numerical Electromagnetics Code (NEC-2) which embodies frequency-domain method and developed to analyze electromagnetic responses of antennas and other metallic structures. On Mark III Hypercube with 32 active nodes, largest lattice contains about 2,048,000 unit cells.
Patterson, J. E.↗
Propagation characteristics of optical fiber structures with arbitrary shape and index variation
The application of the scalar wave-fast Fourier transform (SW-FFT) technique to the computation of the propagation characteristics of some complex optical fiber structures is presented. The SW-FFT technique is based on the numerical solution of the scalar wave equation by a forward-marching fast Fourier transform method. This solution yields the spatial configuration of the fields as well as its modal characteristics in and around the guiding structure. The following are treated by the SW-FFT method: analysis of coupled optical fibers and computation of their odd and even modes and coupling length; the solution of tapered optical waveguides (transitions) and the study of the effect of the slope of the taper on mode conversion; and the analysis of branching optical fibers and demonstration of their mode-filtering and/or power-dividing properties.
Manshadi, F.↗
Designing A Microwave Band-Stop Filter
Lumped-circuit design techniques applied to iris-coupled cavities. Waveguide/cavity filter imitates lumped series and parallel combinations of inductance and capacitance over narrow stopband centered at 7.190 GHz. Filter made of standard WR125 waveguide stock.
Manshadi, F.↗
Compound-taper feedhorn for the DSN 70-meter antennas
A novel X-band feedhorn was designed for the Deep Space Network (DSN) 70-meter antennas. The feedhorn is a compound-taper structure consisting of a corrugated flared section and a corrugated straight section. This feedhorn is designed to closely initiate the characteristics of the standard feedhorn, while providing the proper phase center location, without adding any significant loss to the system. The use of the existing feedhorn and the ease of manufacturing the corrugated straight section have resulted in major overall cost savings.
Manshadi, F.↗