CARACTERIZACION DEL ENTORNO METEORICO DEL SISTEMA TIERRA-LUNA: DETERMINACION DE PROPIEDADES FISICO-QUIMICAS DE METEOROIDES Y DE SU FLUJO DE IMPACTOS
PID2019-105797GB-I00
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Nombre agencia financiadora Agencia Estatal de Investigación
Acrónimo agencia financiadora AEI
Programa Programa Estatal de Generación de Conocimiento y Fortalecimiento Científico y Tecnológico del Sistema de I+D+i
Subprograma Subprograma Estatal de Generación de Conocimiento
Convocatoria Proyectos I+D
Año convocatoria 2019
Unidad de gestión Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020
Centro beneficiario UNIVERSIDAD DE HUELVA
Identificador persistente http://dx.doi.org/10.13039/501100011033
Publicaciones
Resultados totales (Incluyendo duplicados): 1
Encontrada(s) 1 página(s)
Encontrada(s) 1 página(s)
Seismic Observation and Location of a Meteor Burst From a Dense Station Deployment in Southern Spain
Digital.CSIC. Repositorio Institucional del CSIC
- Stich, Daniel
- Casado Rabasco, Josué
- Madiedo, José M.
- Guerrero Rascado, Juan Luis
- Morales Soto, Jose
This is an open access article under the terms of the Creative Commons Attribution-NonCommercial-NoDerivs License, which permits use and distribution in any medium, provided the original work is properly cited, the use is non-commercial and no modifications or adaptations are made., A meteor event on 11 December 2016 in southern Spain was accompanied by an audible boom and felt vibrations. Acousto-seismic coupling of the near-field pressure wave has been recorded by an unusually large number of 44 local seismic stations. Considering the ERA5 atmospheric temperature and wind speed model, we can attribute the seismic detections to a point source at 38 km height, coincident with the most luminous fragmentation event recorded by meteor cameras. We show and analyze waveforms, spectrograms and signal polarization along a dense, temporary broadband transect in the area. Seismic records show important differences between them, like large variability in polarization, amplitudes and frequency content, emphasizing the role of local effects. The duration and complexity of waveforms can be attributed to path and site effects, including multipathing through small-scale atmospheric heterogeneity and scattering of the incoming acoustic wavefield at local topography. © 2022. The Authors., We want to thank the developers of free software BAM (McFadden et al., 2021), ObsPy (Megies et al., 2011), SAC (Goldstein et al., 2003), and GMT (Wessel et al., 2019). We particularly appreciate the help by Luke McFadden with usage and parameter choices in BAM. We thank the IGN for sharing data from the Spanish broadband network, and all staff and students from IAG involved in the deployment and maintenance of the Tropical Profile. We receive financial support by Spanish projects CGL2015-67130-C2-2-R, A-RNM-421-UGR18, PID2019-109608GB-I00, PID2019-105797GB-I00 and B-RNM-528-UGR20., Peer reviewed