Nonparametric H Density Estimation Based on Regularized Nonlinear Inversion of the Lyman Alpha Emission in Planetary Atmospheres

Jianqi Qin, Brian J. Harding, Lara Waldrop

Research output: Contribution to journalArticle

Abstract

Inversion of space-borne remote sensing measurements of the resonantly scattered solar Lyman alpha (121.6-nm) emission in planetary atmospheres is the most promising means of quantifying the H density in a vast volume of space near terrestrial planets. Owing to the highly nonlinear nature of the inverse problem and the lack of sufficient data constraints over the large volume of space where H atoms are present, previous inversion methods relied on physics-based parametric formulations of the H density distributions to guarantee solution uniqueness. Those physical formulations, such as the Chamberlain model, were developed with simple assumptions of the atmospheric conditions. The use of such formulations as constraints significantly limits the range of possible solutions, which might lead to large errors in the case when those assumptions are invalid. In this study, we demonstrate for the first time the feasibility of estimating the H density through regularized nonlinear inversion of the Ly-α emission in an optically thick atmosphere, without using parametric formulations. Specifically, Occam's inversion algorithm is used to demonstrate that the H density can be estimated in a large volume of space near the planet, with accuracy in different atmospheric regions depending on the observation scheme. Two distinctly different schemes are examined, including a low-Earth orbit and a geostationary orbit. Modeling results show that the low-Earth orbit is better for H density estimation in the thermosphere, while the high-altitude orbit is better for estimation in the exosphere. Our results could provide useful information for designing the observation schemes of future missions.

Original languageEnglish (US)
Pages (from-to)8641-8648
Number of pages8
JournalJournal of Geophysical Research: Space Physics
Volume123
Issue number10
DOIs
StatePublished - Oct 2018

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planetary atmosphere
planetary atmospheres
orbits
Orbits
inversions
formulations
low Earth orbits
Planets
Earth (planet)
exosphere
planet
terrestrial planets
thermosphere
high altitude
meteorology
uniqueness
Inverse problems
density distribution
remote sensing
planets

Keywords

  • H density distribution
  • Lyman alpha emission
  • planetary atmospheres
  • radiative transfer
  • regularized nonlinear inversion
  • remote sensing

ASJC Scopus subject areas

  • Geophysics
  • Forestry
  • Oceanography
  • Aquatic Science
  • Ecology
  • Water Science and Technology
  • Soil Science
  • Geochemistry and Petrology
  • Earth-Surface Processes
  • Atmospheric Science
  • Earth and Planetary Sciences (miscellaneous)
  • Space and Planetary Science
  • Palaeontology

Cite this

Nonparametric H Density Estimation Based on Regularized Nonlinear Inversion of the Lyman Alpha Emission in Planetary Atmospheres. / Qin, Jianqi; Harding, Brian J.; Waldrop, Lara.

In: Journal of Geophysical Research: Space Physics, Vol. 123, No. 10, 10.2018, p. 8641-8648.

Research output: Contribution to journalArticle

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