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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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https://doi.org/10.5194/angeo-2019-47
© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/angeo-2019-47
© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.

  28 Mar 2019

28 Mar 2019

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A revised version of this preprint is currently under review for the journal ANGEO.

Inferring thermospheric composition from ionogram profiles: A calibration with the TIMED spacecraft

Christopher J. Scott, Shannon Jones, and Luke A. Barnard Christopher J. Scott et al.
  • Department of Meteorology, University of Reading, Reading, RG6 6BB, UK

Abstract. Measurements of thermospheric composition via ground-based instrumentation are challenging to make and so details about this important region of the upper atmosphere are currently sparse. We present a technique that deduces quantitative estimates of thermospheric composition from ionospheric data, for which there is a global network of stations. The visibility of the F1 peak in ionospheric soundings from ground-based instrumentation is a sensitive function of thermospheric composition. The ionospheric profile in the transition region between F1 and F2 peaks can be expressed by the G factor, a function of ion production rate and loss rates via ion-atom interchange reactions and dissociative recombination of molecular ions. This in turn can be expressed as the square of the ratio of ions lost via these processes. We compare estimates of the G factor obtained from ionograms recorded at Kwajalein (9° N, 167.2° E) for 25 times during which the TIMED spacecraft recorded approximately co-located measurements of the neutral thermosphere. We find a linear relationship between √G and the molecular: atomic composition ratio, with a gradient of 2.23 ± 0.17 and an offset of 1.66 ± 0.19. This relationship reveals the potential for using ground-based ionospheric measurements to infer quantitative variations in the composition of the neutral thermosphere. Such information can be used to investigate spatial and temporal variations in thermospheric composition which in turn has applications such as understanding the response of thermospheric composition to climate change and the efficacy of the upper atmosphere on satellite drag.

Christopher J. Scott et al.

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Christopher J. Scott et al.

Christopher J. Scott et al.

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Latest update: 24 Oct 2020
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Short summary
The composition of the upper atmosphere has been difficult to measure with localised observations relying on spacecraft or sub-orbital rockets or measurements of airglow from ground-based observatories. The height profile of ionisation within the neutral upper atmosphere is influenced by the composition of the neutral gas. We present a method for determining the neutral upper atmosphere composition from measurements of the ionisation profile, and compare these with spacecraft measurements.
The composition of the upper atmosphere has been difficult to measure with localised...
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