Analysis of the September ∈-Perseid outburst in 2013

We analyse the outburst experienced by the September ∈-Perseid meteor shower on 2013 September 9. As a result of our monitoring, the atmospheric trajectory of 60 multistation events observed over Spain was obtained and accurate orbital data were derived from them. On the basis of these orbits, we ha...

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Detalles Bibliográficos
Autores: Madiedo, José M., Zamorano, J., Trigo-Rodríguez, Josep María, Ortiz, José Luis, Docobo, J.A., Izquierdo, J., Lacruz, J., Campo, Pedro P., Andrade, Manuel, Pastor, S., Reyes, J. A. de los, Ocaña, F., Sánchez de Miguel, A., Pujols, P.
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2018
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/194859
Acceso en línea:http://hdl.handle.net/10261/194859
Access Level:acceso abierto
Palabra clave:Meteoroids
Meteors
Meteorites
Descripción
Sumario:We analyse the outburst experienced by the September ∈-Perseid meteor shower on 2013 September 9. As a result of our monitoring, the atmospheric trajectory of 60 multistation events observed over Spain was obtained and accurate orbital data were derived from them. On the basis of these orbits, we have tried to determine the likely parent body of this meteoroid stream by employing orbital dissimilarity criteria. In addition, the emission spectra produced by two events belonging to this meteor shower were also recorded. The analysis of these spectra has provided information about the chemical nature of their progenitor meteoroids. We also present an estimation of the tensile strength for these particles.© 2018 The Author(s).

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