Superconducting Technology Assessment - nitrd
Superconducting Technology Assessment - nitrd
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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