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ORIGINAL RESEARCH article

Front. Astron. Space Sci.

Sec. Space Physics

This article is part of the Research TopicLarge Long-Lived Vertical Wind Oscillations in the Mesosphere and Thermosphere RegionsView all 6 articles

Resolving Thermospheric Vertical Wind Ambiguities and Energy Processes

Provisionally accepted
Jeffrey  P ThayerJeffrey P Thayer*Austin  ColemanAustin Coleman
  • University of Colorado Boulder, Boulder, United States

The final, formatted version of the article will be published soon.

This study applies a generalized vertical coordinate system approach alongside thermodynamic control volume analysis to explore the nuanced interpretations of energy transfer processes associated with vertical motion in the thermosphere. Using simulations from the TIEGCM V3.0 model, a key finding reveals that transforming vertical winds in height coordinates onto constant pressure surfaces contain a substantial lifting component—an aspect often overlooked in previous research. This distinction is critical for internal energy assessments, as vertical winds defined in pressure coordinates directly contribute to the adiabatic heating/cooling rate while only a portion of the vertical wind in height coordinates contributes to these energy changes. These differences are demonstrated through schematic representations of thermodynamic control volumes that model a column of thermospheric gas undergoing various energy transfer processes. Accurately determining the portion of observed vertical winds that affect internal energy requires clear understanding between height and pressure surfaces – a nontrivial challenge in observational contexts. Furthermore, applying the generalized vertical coordinate framework to airglow emissions in the upper thermosphere uncovers an inherent ambiguity: vertical winds inferred from airglow observations may not align with those defined on pressure or height surfaces. This insight suggests that discrepancies in the behavior and magnitude of vertical winds derived from FPI observations of red-line emissions in the upper thermosphere are due to poorly known relations between the emission structure relative to pressure or height surfaces.

Keywords: adiabatic, airglow, Energy, thermosphere, winds

Received: 25 Aug 2025; Accepted: 05 Jan 2026.

Copyright: © 2026 Thayer and Coleman. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) or licensor are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.

* Correspondence: Jeffrey P Thayer

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