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Weimer, D. R., Mlynczak, M. G., Emmert, J. T., Doornbos, E., Sutton, E. K., and Hunt, L. A., 2018. Correlations Between the Thermosphere's Semiannual Density Variations and Infrared Emissions Measured With the SABER Instrument. Journal of Geophysical Research (Space Physics), 123(10):8850–8864, doi:10.1029/2018JA025668.
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@ARTICLE{2018JGRA..123.8850W,
author = {{Weimer}, D.~R. and {Mlynczak}, M.~G. and {Emmert}, J.~T. and {Doornbos}, E. and {Sutton}, E.~K. and {Hunt}, L.~A.},
title = "{Correlations Between the Thermosphere's Semiannual Density Variations and Infrared Emissions Measured With the SABER Instrument}",
journal = {Journal of Geophysical Research (Space Physics)},
keywords = {thermospheric dynamics, thermosphere composition, semiannual variation, satellite drag, thermosphere emissions},
year = 2018,
month = oct,
volume = {123},
number = {10},
pages = {8850-8864},
abstract = "{This paper presents measurements of the amplitudes and timings of the
combined, annual, and semiannual variations of thermospheric
neutral density, and a comparison of these density variations
with measurements of the infrared emissions from carbon dioxide
and nitric oxide in the thermosphere. The density values were
obtained from measurements of the atmospheric drag experienced
by the Challenging Minisatellite Payload, Gravity Recovery and
Climate Experiment A, Gravity field and Ocean Circulation
Explorer, and three Swarm satellites, while the optical
emissions were measured with the Sounding of the Atmosphere
using Broadband Emission Radiometry (SABER) instrument on the
Thermosphere Ionosphere Mesosphere Energetics and Dynamics
satellite. These data span a time period of 16 years. A database
containing global average densities that were derived from the
orbits of about 5,000 objects (Emmert, 2009, <A href=``https://d
oi.org/10.1029/2009JA014102''>https://doi.org/10.1029/2009JA0141
02</A>, 2015b, <A href=``https://doi.org/10.1002/2015JA021047''>
https://doi.org/10.1002/2015JA021047</A>) was employed for
calibrating these density data. A comparison with the
NRLMSISE-00 model was used to derive measurements of how much
the density changes over time due to these seasonal variations.
It is found that the seasonal density oscillations have
significant variations in amplitude and timing. In order to test
the practicality of using optical emissions as a monitoring
tool, the SABER data were fit to the measured variations. Even
the most simple fit that used only filtered carbon dioxide
emissions had good correlations with the measured oscillations.
However, the density oscillations were also well predicted by a
simple Fourier series, contrary to original expectations.
Nevertheless, measurements of the optical emissions from the
thermosphere are expected to have a role in future understanding
and prediction of the semiannual variations.}",
doi = {10.1029/2018JA025668},
adsurl = {https://ui.adsabs.harvard.edu/abs/2018JGRA..123.8850W},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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