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Comparison of GOLD nighttime measurements of OI 135.6 nm radiance with the total electron content map: preliminary results
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  • Xuguang Cai,
  • Alan Burns,
  • Wenbin Wang,
  • Anthea Coster,
  • Liying Qian,
  • Jing Liu,
  • Stanley Solomon,
  • Richard Eastes,
  • Robert Daniell,
  • William McClintock
Xuguang Cai
University Corporation for Atmospheric Research

Corresponding Author:[email protected]

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Alan Burns
National Center for Atmospheric Research
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Wenbin Wang
High Altitude Observatory
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Anthea Coster
MIT Haystack Observatory
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Liying Qian
University Corporation for Atmospheric Research
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Jing Liu
National Center for Atmospheric Research
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Stanley Solomon
National Center for Atmospheric Research
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Richard Eastes
Laboratory for Atmospheric and Space Physics
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Robert Daniell
Ionospheric Physics
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William McClintock
Laboratory for Atmospheric and Space Physics
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Abstract

The unambiguous 2-dimensional (2D) maps of OI 135.6 nm radiance retrieved from the Global Observation of Limb and Disk (GOLD) after sunset are compared with the total electron content (TEC) maps measured by GPS receivers in the America sector. The OI 135.6 nm radiance observed by GOLD is an indicator of the peak electron density of the ionosphere, while the TEC depends on the total electron density in the column. The comparisons show that both of them are able to capture the large structures in the equatorial ionization anomaly (EIA) well, and sometimes they both also capture bubbles. Both show that the ionosphere after sunset is quite dynamic and has strong day-to-day variability. A statistical study has also been carried out to check the occurrence rate of bubbles and the apparent EIA structure between Oct 17, 2018 to May 31, 2019. GOLD is able to image the areas where it is difficult to situate GPS receivers such as the ocean, while TEC data covers the full-diurnal cycle. In all, the GOLD and TEC have valuable synergy to allow us to gain a better understanding of the equatorial ionosphere.