9–13 Sept 2024
Turin, Italy
Europe/Rome timezone

Observations and Numerical Simulations of the Effects of the Gamma Ray Burst 221009A on the Lower Ionosphere

Not scheduled
1h
Turin, Italy

Turin, Italy

Centro Congressi Unione Industriali Torino Via Vela, 17 - 10128 Torino
Poster Space weather and the solar-heliospheric connections Coffee break and poster session 2

Description

In this contribution we investigated the impact of a powerful gamma ray burst (GRB) that
occurred on October 9 2022, on the Earth's environment using a very low frequency
receiver (VLF) to probe the lower ionospheric region (the D region). In addition to the
VLF data analysis, we employed numerical simulation through the Long Wavelength
Propagation Capability code (LWPC) to derive the increase in the D-region electron
density. Our results revealed discernible perturbations in amplitude and phase across all
transmitter paths (NAA, DHO, ICV, and NSC) to the Algiers receiver persisting for 40
minutes. At the maximum of the signal perturbation, the LWPC simulation results showed
a decrease in the mean new reference height h’ from 74 km to 65.71 km, along with an
increase in the sharpness factor $\beta$ from 0.3 km-1 to 0.4875 km-1. Under these new
conditions, the electron density increased from its ambient value (216.10 cm-3 to 33.7 103
cm-3

Primary authors

Samir NAIT AMOR (Center for Research in Astronomy Astrophysics and Geophysics (CRAAG)) Mrs Fethia Kerrache Dr Ahmed Ammar (ESPRIT School of Engineering and LSAMA Laboratory, Faculty of Sciences) Dr Rabah Ikhlef (Center for Research in Astronomy Astrophysics and Geophysics (CRAAG)) Dr Khalil Daifellah (Center for Research in Astronomy Astrophysics and Geophysics (CRAAG)) Dr Zineddine Bouyahiaoui (Center for Research in Astronomy Astrophysics and Geophysics (CRAAG))

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