Geomagnetic and ionospheric effects two consecutive strong earthquakes in Morocco on september 08, 2023
- Autores: Adushkin V.V.1, Spivak A.A.1, Riabova S.A.1, Tikhonova A.V.1
- 
							Afiliações: 
							- Sadovsky Institute of Geosphere Dynamics of Russian Academy of Sciences
 
- Edição: Volume 515, Nº 1 (2024)
- Páginas: 118-123
- Seção: SEISMOLOGY
- ##submission.dateSubmitted##: 31.01.2025
- ##submission.datePublished##: 30.09.2024
- URL: https://hum-ecol.ru/2686-7397/article/view/649968
- DOI: https://doi.org/10.31857/S2686739724030144
- ID: 649968
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		                                					Resumo
The geophysical effects of a strong seismic event in the form of two earthquakes of magnitude 6.8 and 4.9 that occurred on September 08, 2023 in Morocco at close times 22:11 and 22:30 UTC with an epicentral distance between the foci of ~ 4 km are considered. We used data from a number of observatories of the INTERMAGNET network and the results of magnetic registration at the Mikhnevo Geophysical Observatory of IDG RAS. It was shown that in the absence of significant global disturbances of the Earth’s magnetic field, earthquakes were accompanied by a series of three positive bay-shaped geomagnetic variations with maximum amplitudes from ~1 to ~10 nT, following each other after ~60 min. The maxima of the induced magnetic field variations were observed almost synchronously at distances from ~800 to ~10000 km. The delay time of the magnetic effect relative to the main shock of the first earthquake was ~70 min. Taking into account the almost planetary nature and high synchronicity of the magnetic field disturbances caused over a significant range of distances, as well as time delays corresponding in order of magnitude to the travel time of the seismic signal of a distance multiple of the size of the Earth, it is suggested that the magnetic effect of the seismic event in question was caused by a global source, which can serve as an excited geodynamo. The ionospheric effect of the seismic event under consideration is presented in the form of variations of the critical frequency f0F2 calculated from the data of the ground-based sounding station of the del Ebre Observatory.
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	                        Sobre autores
V. Adushkin
Sadovsky Institute of Geosphere Dynamics of Russian Academy of Sciences
														Email: aaspivak100@gmail.com
				                					                																			                								
Academician of the RAS
Rússia, MoscowA. Spivak
Sadovsky Institute of Geosphere Dynamics of Russian Academy of Sciences
							Autor responsável pela correspondência
							Email: aaspivak100@gmail.com
				                					                																			                												                	Rússia, 							Moscow						
S. Riabova
Sadovsky Institute of Geosphere Dynamics of Russian Academy of Sciences
														Email: riabovasa@mail.ru
				                					                																			                												                	Rússia, 							Moscow						
A. Tikhonova
Sadovsky Institute of Geosphere Dynamics of Russian Academy of Sciences
														Email: aaspivak100@gmail.com
				                					                																			                												                	Rússia, 							Moscow						
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