Quantification of Perturbation to the Daytime Lower Ionosphere From a Gamma Ray Burst Using ELF Remote Sensing

Abstract On 9 October 2022, a powerful gamma ray burst (GRB), GRB221009A, caused significant changes in the electron density of the lower ionosphere, as evidenced by VLF (3–30 kHz) radio wave observations. However, GRB221009A did not yield any observable signatures at the Schumann resonances (∼8, ∼14 Hz), which are also sensitive to the lower ionosphere. We show that the effects of GRB221009A are observable in a decrease in propagation velocity of ELF (3–1,000 Hz) lightning impulses. Analytical and numerical analysis points to an ionospheric perturbation in which the GRB increased the daytime electron density uniformly over a wide altitude range from 50 to 90 km. The GRB perturbation is markedly different from perturbations from solar flares, which significantly increase the vertical gradient of the electron density. ELF propagation velocity is shown to be a technique that can identify the altitude range of ionospheric perturbations.

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Publication Details

Journal
Geophysical Research Letters
Published
2025-11-11
DOI
https://doi.org/10.1029/2025gl117989
Primary Topic
Gamma-ray bursts and supernovae
Type
article
Field-Weighted Citation Impact
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article

Quantification of Perturbation to the Daytime Lower Ionosphere From a Gamma Ray Burst Using ELF Remote Sensing

János Lichtenberger, Zenon Nieckarz, Mark Gołkowski, Andrew Klekociuk et al.
Geophysical Research Letters
Gamma-ray bursts and supernovae
article

Quantification of Perturbation to the Daytime Lower Ionosphere From a Gamma Ray Burst Using ELF Remote Sensing

János Lichtenberger, Zenon Nieckarz, Mark Gołkowski, Andrew Klekociuk, M. Ostrowski, A. Michalec, P. Nicholson, Janusz Młynarczyk, Jerzy Kubisz
article en

Abstract

Abstract On 9 October 2022, a powerful gamma ray burst (GRB), GRB221009A, caused significant changes in the electron density of the lower ionosphere, as evidenced by VLF (3–30 kHz) radio wave observations. However, GRB221009A did not yield any observable signatures at the Schumann resonances (∼8, ∼14 Hz), which are also sensitive to the lower ionosphere. We show that the effects of GRB221009A are observable in a decrease in propagation velocity of ELF (3–1,000 Hz) lightning impulses. Analytical and numerical analysis points to an ionospheric perturbation in which the GRB increased the daytime electron density uniformly over a wide altitude range from 50 to 90 km. The GRB perturbation is markedly different from perturbations from solar flares, which significantly increase the vertical gradient of the electron density. ELF propagation velocity is shown to be a technique that can identify the altitude range of ionospheric perturbations.

Geophysical Research LettersVol. 52(22)
Obuda University (HU), Eötvös Loránd University (HU), Jagiellonian University (PL), Institute of Physics (PL), Turkish Ophthalmological Association (TR), The University of Adelaide (AU), AGH University of Krakow (PL), University of Colorado Denver (US)
National Science Foundation, Narodowym Centrum Nauki, University of Colorado Denver
Openalex Percentile: Top 77%
Gamma-ray bursts and supernovae
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