SH013-11
Comparing numerical models to laboratory experiment results using the twin-probe method: a technique to improve Langmuir probe measurement accuracy on very small satellites
Abstract:
Numerical simulations and plasma laboratory experiments were conducted to study the TPM’s efficacy and maximize its impact. The experiments took place at NASA Marshall Space Flight Center and studied changes to the S/C potential during LP operation using the TPM in an approximated low Earth orbit (LEO) plasma environment. Results from this experiment were exhibited in the 2019 AGU Fall Meeting [1]. Additionally, the Plasma-Spacecraft Interaction Codes for Low Earth Orbit (PSIC-LEO) were developed at the University of Michigan to model the induced S/C potential due to LP operation using analytic expressions and to understand its effects on LP current-voltage characteristics. Here we present comparisons between experimental results and simulation predictions with a focus on electron temperature and density measurement correction when varying the spacecraft-to-LP area ratio. Generally, the model predictions and experimental results agree on TPM measurement corrections to within 5%. Additionally, both simulation and experiment efforts show greater corrections to LP electron density and temperature measurements as the area ratio decreases. Finally, we will use the lessons learned from these research initiatives to highlight additional applications for a twin-probe system on a CubeSat platform, such as maintaining a negative CubeSat potential to enhance ion energy analyzer performance.
[1] Leon, Omar, et al. "The twin-probe method: tracking the variable potential of small satellites to improve Langmuir probe measurement accuracy." AGUFM 2019 (2019): A41U-2688.