Comparison of GOLD Nighttime Measurements With Total Electron Content: Preliminary Results
Name
JGR Space Physics - 2020 - Cai - Comparison of GOLD Nighttime Measurements With Total Electron Content Preliminary Results.pdf
Description
Published version
Size
14.13 MB
Format
Adobe PDF
Checksum (MD5)
29a6224335e222e75cec7651d5560810
Author(s)
Cai, Xuguang
Burns, Alan G
Wang, Wenbin
Coster, Anthea
Qian, Liying
Liu, Jing
Solomon, Stanley C
Eastes, Richard W
Daniell, Robert E
McClintock, William E
Date Issued
August 24, 2020
Journal
Journal of Geophysical Research: Space Physics
Publisher
American Geophysical Union
Citation
Cai, X., Burns, A. G., Wang, W., Coster, A., Qian, L., & Liu, J., et al. (2020). Comparison of GOLD nighttime measurements with total electron content: Preliminary results. Journal of Geophysical Research: Space Physics, 125, e2019JA027767.
Version
Final published version
Abstract
The National Aeronautics and Space Administration (NASA) Global‐scale Observations of the Limb and Disk (GOLD) has been imaging the thermosphere and ionosphere since October 2018. It provides continuous measurements over a large area from its geostationary orbit. The unambiguous two‐dimensional (2‐D) maps of OI 135.6 nm radiance retrieved from GOLD after sunset are compared with the total electron content (TEC) maps measured by GPS receivers in the American sector. The OI 135.6 nm radiance observed by GOLD is an indicator of the peak electron density of the ionosphere F2 region, while the TEC is the total electron density in the column. Our comparisons show that the two data sets match each other very well in the equatorial ionization anomaly (EIA) morphology and its seasonal variability. Equatorial plasma bubbles (EPBs) are evident in GOLD nighttime OI 135.6 radiance. Corresponding depletions are shown in TEC maps, but without GOLD data as a reference, it is difficult to discern that the depletions are EPBs. In addition, both GOLD 135.6 radiance and TEC maps observed third peaks of electron density poleward of the southern EIA crests. Furthermore, both show that the ionosphere after sunset is quite dynamic and has strong day‐to‐day variability. In all, the GOLD and TEC have valuable synergy to allow us to gain a better understanding of the equatorial ionosphere.
MIT Department
Haystack Observatory
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Persistent DSpace Link
DOI of Published Version
https://doi.org/10.1029/2019ja027767
