Chemical heat derived from rocket-borne WADIS-2 experiment

Abstract Chemical heating rates were derived from three of the most significant reactions based on the analysis of common volume rocket-borne measurements of temperature, atomic oxygen densities, and neutral air densities. This is one of the first instances of the retrieval of nighttime chemical heat through the utilization of non-emissive observations of atomic oxygen concentrations, obtained through in situ measurements, performed at the Andøya Space Center (69°N, 16°E) at 01:44:00 UTC on 5 March 2015. Furthermore, we determine the heating efficiency for one of the most significant reactions of atomic hydrogen with ozone and illustrate the methodology for such calculations based on known atomic oxygen and temperature. Subsequently, using ozone values obtained from satellite observations, we retrieved odd-hydrogens and total chemical heat. Finally, we compared the retrieved chemical heat with the heat from turbulent energy dissipation. Our findings reveal that the vertically averaged chemical heat is greater than the heat from turbulent energy dissipation throughout the entire mesopause region during nocturnal conditions. The heating rates of turbulent energy dissipation may exceed the chemical heating rates only in narrow peaks, several hundred meters wide. Graphical Abstract

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Publication Details

Journal
Earth Planets and Space
Published
2024-12-30
DOI
https://doi.org/10.1186/s40623-024-02129-x
Citations
3
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
0.99

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article

Chemical heat derived from rocket-borne WADIS-2 experiment

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3 citations
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Ionosphere and magnetosphere dynamics
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article

Chemical heat derived from rocket-borne WADIS-2 experiment

Boris Strelnikov, Claudia Stephan, M. Grygalashvyly, Irina Strelnikova, Martin Eberhart, Stefanos Fasoulas, Markus Rapp, Franz‐Josef Lübken, Stefan Löhle, Corinna Schütt
article en
3 citations

Abstract

Abstract Chemical heating rates were derived from three of the most significant reactions based on the analysis of common volume rocket-borne measurements of temperature, atomic oxygen densities, and neutral air densities. This is one of the first instances of the retrieval of nighttime chemical heat through the utilization of non-emissive observations of atomic oxygen concentrations, obtained through in situ measurements, performed at the Andøya Space Center (69°N, 16°E) at 01:44:00 UTC on 5 March 2015. Furthermore, we determine the heating efficiency for one of the most significant reactions of atomic hydrogen with ozone and illustrate the methodology for such calculations based on known atomic oxygen and temperature. Subsequently, using ozone values obtained from satellite observations, we retrieved odd-hydrogens and total chemical heat. Finally, we compared the retrieved chemical heat with the heat from turbulent energy dissipation. Our findings reveal that the vertically averaged chemical heat is greater than the heat from turbulent energy dissipation throughout the entire mesopause region during nocturnal conditions. The heating rates of turbulent energy dissipation may exceed the chemical heating rates only in narrow peaks, several hundred meters wide. Graphical Abstract

Earth Planets and SpaceVol. 76(1)
University of Stuttgart (DE), Deutsches Zentrum für Luft- und Raumfahrt e. V. (DLR) (DE), Leibniz Institute of Atmospheric Physics at the Rostock University (DE), University of Rostock (DE)
Deutsches Zentrum für Luft- und Raumfahrt
Affordable and clean energy
Openalex Percentile: Top 22%
Ionosphere and magnetosphere dynamics
0.99
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