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Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
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A W-Band HEMT Based Power Amplifier Module for Millimeter-Wave LO Multiplier
We report on the performance of power amplifiers as local oscillator drivers for millimeter and submillimeter-wave receivers.
A 294 GHz 0.47m W Caterpillar amplifier based transmitter in 65 nm CMOS for THz data-links
A fully integrated CMOS THz transmitter for short range data-links is presented which provides 0.47 mW of output power to 294 GHz. The output frequency is derived from a 147 GHz on-chip LO and fully differential caterpillar power amplifier combined with a transformer coupled frequency doubler. The transmitter is integrated with an on-chip dipole antenna for use in THz communication systems and consumes a total of 258 mW.
Insitu Lunar Launch & Landing Pad Construction w/ Regolith and Thermoset Polymers
This CIF project is an extension of materials developed under a previous NASA Innovative Advanced Concepts (NIAC) project titled “Regolith Derived Heat Shield for Planetary Body Entry and Descent Systems with In-Situ Fabrication” by M. Hogue et al. (2012). Launch and landing pads are necessary to mitigate risks to lander/ascent vehicles, surface assets, and orbital assets from rocket plume ejected regolith. At this time, all launching and landing on the lunar surface will be on unprepared surface sites. Though this has been a successful approach for Apollo and other uncrewed missions, significant risks exist for the Artemis Program due to the increased thrust of the vehicles, presence of co-located assets, and potential surface level requirements for tall vehicles. This project developed a thermoset polymer–regolith composite material for use as a launch and landing pad. Test articles were prepared at 20% and 11% polymer mass percent (wt%) and tested under hot fire conditions that simulated large vehicle lunar launch/landing conditions. A minimum polymer wt% of 9% was achieved and both samples successfully mitigated regolith ejecta from plume effects. A concept for emplacing launch/landing pads was successfully tested in laboratory environments using a screw and barrel approach to mixing, conveying and depositing materials. It is recommended that materials and systems be developed to TRL 6 for a small-scale lunar demonstration of emplacement of a launch/landing pad via a Commercial Lunar Payload Services (CLPS) mission to support the Artemis Program.
Hot Hydrogen Testing of W-coated UN Kernels for Nuclear Thermal Propulsion
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Characterization of a 50 W Tuned Inductance Linear Alternator and Controller
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The Composition of ~96 keV W+ in Saturn’s Magnetosphere
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Transpressional Rupture Cascade of the 2016 M w 7.8 Kaikoura Earthquake, New Zealand
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Photometric observations of the W UMa stars CSS J113505.5+332031, ASAS J142124+1813.1 and HR Boo
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Energetic Ion Injections Inside Geosynchronous Orbit: Convection‐ and Drift‐Dominated, Charge‐Dependent Adiabatic Energization ( W = qEd )
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Statistical Significance of Precursory Gravity Changes Before the 2011 M w 9.0 Tohoku‐Oki Earthquake
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Characterization of a 10 W class electrospray array thruster
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Interannual Variability of Winds in the Antarctic Mesosphere and Lower Thermosphere Over Rothera (67°S, 68°W) During 2005–2021 in Meteor Radar Observations and WACCM‐X
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First observations of W Virginis stars with K2: detection of period doubling
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A novel survey for young substellar objects with the W -band filter III: Searching for very low-mass brown dwarfs in Serpens South and Serpens Core
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The effect of resting blood flow occlusion on exercise tolerance and W′
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Tectonic inversion in the Caribbean-South American plate boundary: GPS geodesy, seismology, and tectonics of the M w 6.7 22 April 1997 Tobago earthquake
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