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COSMIAC is working under sponsorship
of the National Science Foundation's Research
for Engineering Undergraduates (REU) program
to develop research interest for undergraduates.
DotSat Ionospheric RF Dispersion Instrument
When radio signals hit the earth's ionosphere, they are bent in a fashion that either reflects them or can cause them to be delayed depending upon frequency. This is particularly important for GPS systems because they must transit the ionosphere to reach the earth, and because their timing is critical to ensure GPS accuracy.
COSMIAC is currently designing an tiny, very inexpensive instrument that will allow scientists to make detailed soundings of the ionosphere using signals from natural transients such as lightning storms. The work is sponsored by the National Science Foundation's Research experiences for Undergraduates (REU) program.
Science Goals:
DotSat is intended to shed light on:
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Total
Electron Content (TEC), magnetic field
strength, refractive effects, plasma properties,
and higher-order electron density profile
effects; |
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Relationships
between lightning effects and thunderstorm
weather in the troposphere; and |
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The potential
relationship between the acoustic/seismic
events around thunderstorms and ionospheric
weather. |
What's Unique about DotSat
Previous missions have made measurements on ionospheric dispersion by observing RF signals from lightning and other transients. Although they were much higher quality instruments than DotSat, they could not locate the source of the lightning observed and therefore could not determine the entire geometry to solve for the ionospheric effects. DotSat will change this completely by using an array of low-cost detectors with precision timing, some on the ground and one in space. These will be used to reference geometrical information for the space-based spectrometer that will make the key soundings. The result will be a complete view of the dispersion process.
The REU Team
DotSat is unusual in that it is primarily being designed and built by undergraduate engineering and science students. Although the design of the instrument is a complex state-of-the-art challenge, it is within the grasp of a well-balanced, carefully chosen team of undergraduates. This affords the team an unusual opportunity to learn:
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Receiver design,
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High-speed
ADC and digital board design |
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FPGA Design, |
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Microcontroller programming, |
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Circuit analysis,
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Antenna design,
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DSP processing,
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Filter design,
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Power, |
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Communications.
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Phases
This activity will last for three years and is in the process of completing the first phase this summer (2010). The first year goals concern simply making a small, low-cost RF spectrometer system that can capture time domain data in the range of 20-200MHz. The second year will focus on repackaging the system for a suitable ground system that can be replicated. The third year will make the system into flight hardware.
Further Information
Steve Suddarth, Ph.D. (steve.suddarth@cosmiac.org)
http://cosmiac.ece.unm.edu/index.php/Space_Weather |