@conference{10272/9291,
year = {2013},
url = {http://hdl.handle.net/10272/9291},
abstract = {The identification of their progenitor
bodies is crucial to increase our knowledge on the
origin and evolution of meteoroid streams. Traditionally,
the similarity between two orbits has been used to
link a given meteoroid stream with a potential parent
body. This similarity was first expressed in terms of
the so-called D-criterion, which was originally proposed
by Southworth and Hawkins [1]. Alternative
versions of this criterion have been proposed by other
authors [2-5]. In order to establish a relationship between
the orbit of the meteoroids and that of their potential
parent bodies, the availability of precise orbital
parameters is fundamental. Due to the chance of finding
wrong parent body candidates, it is also crucial to
integrate the orbits of the bodies backwards in time to
analyze the evolution of these criteria and to establish
real (not casual) connections [6]. In this work we analyze
a double-station fireball imaged in the framework
of the SPanish Meteor Network (SPMN). By using the
Mercury 6 symplectic integrator [7] and orbital association
software developed by us [8], we have identified
a NEO as the progenitor body of the parent meteoroid.},
title = {Linking a fireball to its likely parent near earth object by means of orbital analysis software tools},
author = {Alonso, C. and Madiedo Gil, José María and Trigo Rodríguez, Josep María and Ortiz Moreno, José Luis and Castro Tirado, Alberto J. and Pastor, S. and Reyes, J. A. de los},
}