Preprints
https://doi.org/10.5194/egusphere-2026-1118
https://doi.org/10.5194/egusphere-2026-1118
27 Mar 2026
 | 27 Mar 2026
Status: this preprint is open for discussion and under review for Annales Geophysicae (ANGEO).

Non-Maxwellian electron distributions in the D region during artificial heating (Paper II): Electron cooling rates

Margaretha Myrvang and Björn Johan Gustavsson

Abstract. This paper investigates how non-Maxwellian distributions of heated electrons modify the macroscopic properties of the electron gas in the D region. Adjusted electron cooling rates for vibrational excitation of molecular nitrogen and molecular oxygen, as well as excitation of fine structure levels in atomic oxygen, are presented. These electron cooling rates are compared to Maxwellian cooling rates from previous studies by Pavlov (1998a), Campbell et al. (2004) , Pavlov (1998b) and Pavlov (1998). We find that the electron cooling rates for vibrational excitation of molecular nitrogen and excitation of fine structure levels in atomic oxygen are more affected by deviations from Maxwellian compared to the cooling rates for vibrational excitation of molecular oxygen. This is due changes in the electron phase space density, where inelastic collision between electrons and neutrals leads to redistribution of electrons.

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Margaretha Myrvang and Björn Johan Gustavsson

Status: open (until 08 May 2026)

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Margaretha Myrvang and Björn Johan Gustavsson
Margaretha Myrvang and Björn Johan Gustavsson
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Short summary
This is the second of two papers. The first paper demonstrate that the electron distribution becomes non-Maxwellian during radio wave heating. Electron cooling rates are macroscopic properties of the electron gas, where electrons transfer some of their kinetic energy through collisions with neutrals and ions, and can be determined by integrating over the electron distribution. Any changes in the electron distribution affect the cooling rates.
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