Abstract
The Dragonfly mission to Titan represents the first use of a large-scale radioisotope power source in that environment; as such little is known of its potential effects on the surface or near-surface atmosphere. These effects represent backgrounds it will be necessary to subtract from the spacecraft's instrumentation data. Repurposing a Monte Carlo code model of the generator built for previous neutronic investigations with the addition of electron detectors allows for the determination of the degree to which the radiation fields from the generator may ionize the surrounding atmosphere and generate interference with the lander's conductivity measurements. Results showed good agreement with experimental data undertaken at the Idaho National Laboratory using the F-2 generator flown on the Perseverance Mars rover, and showed that the interference with readings taken in the daytime on Titan when atmospheric conductivity is expected to be low may be substantial.
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