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On the role of dust in the lunar ionosphere
Authors:TJ Stubbs  DA Glenar  WM Farrell  RR Vondrak  MR Collier  JS Halekas  GT Delory
Institution:aCenter for Research and Exploration in Space Science and Technology, University of Maryland, Baltimore County, MD, USA;bNASA Goddard Space Flight Center, Greenbelt, MD, USA;cNew Mexico State University, Las Cruces, NM, USA;dSpace Sciences Laboratory, University of California, Berkeley, CA, USA;eNASA Ames Research Center, Moffett Field, CA, USA;fNASA Lunar Science Institute, NASA Ames Research Center, Moffett Field, CA, USA
Abstract:Radio occultation measurements from the Soviet Luna 19 mission suggest that electron concentrations above the sunlit lunar surface can be significantly higher than that expected from either the photo-ionization of exospheric neutrals or any other well-known process. These measurements were used to infer the electron column concentrations above the lunar limb as a function of tangent height, which surprisingly indicated peak concentrations of ∼103 cm−3 at ∼5 km altitude. It has been speculated that electrically charged exospheric dust could contribute to such electron populations. This possibility is examined here using the exospheric dust abundances inferred from Apollo 15 coronal photographs to estimate the concentration of electrons produced by photo- and secondary emission from dust. These estimates far exceed the electron concentrations predicted by any other suggested mechanism, and are within a factor of ≈20 of those inferred from the Luna 19 measurements. It is possible that this discrepancy is due to an under-estimate in dust grain capacitances and/or the presence of much higher exospheric dust abundances during the Luna 19 measurements. These results suggest that electrons emitted from exospheric dust could be responsible for the Luna 19 measurements, and that this process could dominate the formation and evolution of the lunar ionosphere.
Keywords:Moon  Lunar ionosphere  Radio occultation  Dust-electrons  Luna 19  Apollo 15  Horizon glow
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