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Superconducting Technology Assessment - nitrd

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In imaging and surveillance systems, most of the data collected tells us that nothing has changed and may be<br />

discarded. Yet many systems are designed to ship all data to the ground for processing in a centralized location,<br />

often introducing a substantial lag time before the useful information is ready. This scheme wastes substantial<br />

bandwidth and transmission power, and reduces the value of the information. Instituting distributed, on-board<br />

processing—especially if software defined and having a “send-everything” option—can deliver the actionable<br />

knowledge contained in the data with better efficiency in terms of time, bandwidth, and power. Superconductive<br />

digital electronics, once matured, should be up to this task.<br />

Deep Space Applications<br />

The cold background temperatures of deep space make the use of superconductive electronics for the entire<br />

receive chain highly attractive. Superconductive antennas can set exceptionally low system noise temperatures.<br />

Superconductive mixers are already the work horse of astrophysical receivers above 100 GHz. And the low noise<br />

temperatures and extreme sensitivity possible in superconductive ADC and following digital filters allow weak<br />

signals to be sensed.<br />

One long-time dream for NASA is a mission to Pluto. Because a lander mission does not appear feasible, a flyby of<br />

perhaps 30 minutes duration is the most likely scenario. With communication lag times of many hours between<br />

Earth and Pluto, the space probe would require fully autonomous data gathering and analysis capabilities. Analysis<br />

during flyby is critical for optimizing the quality of data collected. There is very little hope of providing the power<br />

needed for CMOS-based data processing, but superconducting electronics could provide the processing capabilities<br />

needed at a fraction of the power budget for CMOS.<br />

NASA is actively pursuing a program for missions to the icy moons of Jupiter. Here, the problem for CMOS is both<br />

cold and intense radiation. However, CMOS can be shielded and radiation-hardened, and radioisotope thermoelectric<br />

generators provide both heat and electrical power. Nuclear propulsion is being developed as a key technology and<br />

will provide more electrical power. Given these workarounds, superconducting electronics is not critical for achieving<br />

mission goals; however, RSFQ could provide a boost in computing power and a higher-performance communications<br />

system. This might serve to increase the science return of such missions.<br />

For many years, NASA has been carrying out missions to Mars. Recently, it has committed to an ambitious program<br />

of returning to the moon as a way-station for (potentially manned) travel to Mars. With all this activity, NASA has<br />

come to realize the need for an interplanetary communications network to provide the bandwidth needed for<br />

returning scientific data to Earth. The Mars Telecom Orbiter (MTO), expected to launch in 2009, is intended to<br />

provide some of that bandwidth. Just as superconducting electronics is attractive for use in cellular phone<br />

networks, so, too, it would be attractive in missions similar to the MTO. Additionally, the superconducting analog<br />

of MTO could provide high-performance computing capability for in situ analysis of data.<br />

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