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Mehta, Piyush M., Linares, Richard, and Sutton, Eric K., 2019. Data-Driven Inference of Thermosphere Composition During Solar Minimum Conditions. Space Weather, 17(9):1364–1379, doi:10.1029/2019SW002264.
• from the NASA Astrophysics Data System • by the DOI System •
@ARTICLE{2019SpWea..17.1364M,
author = {{Mehta}, Piyush M. and {Linares}, Richard and {Sutton}, Eric K.},
title = "{Data-Driven Inference of Thermosphere Composition During Solar Minimum Conditions}",
journal = {Space Weather},
year = 2019,
month = sep,
volume = {17},
number = {9},
pages = {1364-1379},
abstract = "{Mass density variations can deviate from the expected behavior caused by
temperature due to changes in the composition. Such deviations
can be especially significant during solar minimum conditions.
Model-data differences are typically resolved through
temperature corrections while overlooking the role of errors in
lower boundary composition. In this work, we use a data-driven
methodology to simultaneously estimate thermosphere composition
and temperature contributions to model-data differences. The
methodology uses modal decomposition to extract high-
dimensional, reduced order basis functions for the covariance of
the neutral thermospheric species and temperature. The extracted
basis functions are combined with CHAllenging Minisatellite
Payload and Gravity Recovery And Climate Experiment mass density
measurements using a nonlinear least squares solver. We
demonstrate the methodology using the Naval Research
Laboratory's empirical Mass Spectrometer and Incoherent Scatter
(MSIS) model to derive the high-dimensional basis functions. We
characterize and quantify the contribution of temperature and
lower boundary effects with oxygen and helium since the two
species have a direct impact on drag and orbit prediction
through gas-surface interactions and mass density. We analyze
the month of December in 2008, based on the work of Thayer et
al. (2012), and estimate that lower boundary composition errors
contribute approximately 50\% of the model-data differences.}",
doi = {10.1029/2019SW002264},
adsurl = {https://ui.adsabs.harvard.edu/abs/2019SpWea..17.1364M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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