Preprints
https://doi.org/10.5194/egusphere-2025-2340
https://doi.org/10.5194/egusphere-2025-2340
28 May 2025
 | 28 May 2025
Status: this preprint is open for discussion and under review for Annales Geophysicae (ANGEO).

Effect of Ionospheric Variability on the Electron Energy Spectrum estimated from Incoherent Scatter Radar Measurements

Oliver Stalder, Björn Gustavsson, and Ilkka Virtanen

Abstract. The ion composition in the E-region is modified by auroral precipitation. This affects the inversion of electron density profiles from field-aligned incoherent scatter radar measurements to differential energy spectra of precipitating electrons. Here a fully dynamic ionospheric chemistry model (IonChem) is developed that integrates the coupled continuity equations for 6 ion and 9 neutral species, modeling the rapid ionospheric variability during active aurora. IonChem is used to produce accurate, time-dependent recombination rates for ELSPEC to improve the inversion of electron density profiles to primary electron energy spectra. The improvement of the dynamic recombination rates on the inversion is compared with static recombination rates from the International Reference Ionosphere (IRI) and the steady-state recombination rates from a ionospheric chemistry model, FlipChem. A systematic overestimation at high electron energies can be removed using a dynamic model. The comparison with FlipChem shows that short-timescale density variations are missed in a steady-state chemistry model

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Oliver Stalder, Björn Gustavsson, and Ilkka Virtanen

Status: open (until 23 Jul 2025)

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Oliver Stalder, Björn Gustavsson, and Ilkka Virtanen
Oliver Stalder, Björn Gustavsson, and Ilkka Virtanen

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Short summary
The rapid changes in ion composition during auroral are dynamically modeled by integrating the coupled continuity equations for 15 ionospheric species. The effect of the ionospheric variation on the inversion of ISR electron density profiles to differential energy spectra of precipitating electrons is studied. A systematic overestimation at high electron energies can be removed using a dynamic model. Comparisons are made with static and steady-state ionospheric models.
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