@conference{10272/9211,
year = {2013},
url = {http://hdl.handle.net/10272/9211},
abstract = {The characterisation of physical and
chemical properties of meteoroids can be performed
from the analysis of meteor and fireball events. This
provides useful information about the origin and evolution
of meteoroid streams and meteoroids of sporadic
origin, but also about the mechanisms that deliver
these materials to the Earth
One of the systems that the SPanish Meteor Network
(SPMN) employs to study the activity of meteor
streams is based on high-sensitivity CCD video cameras.
These devices, which are commonly used to
monitor the night sky, provide useful data for the determination,
for instance, of radiant, orbital and
photometric parameters [1, 2, 3]. They are also very
useful for meteor spectroscopy [3]. As a matter of fact,
the recording and analysis of meteor spectra is one of
the goals of our network, and some of our observing
stations perform a continuous spectroscopic campaign
since 2006. In this context, we analyze here a mag. -10
sporadic fireball recorded from two of our meteor stations
on October 4, 2011.},
title = {Emission spectrum and orbital elements of a sporadic fireball imaged in 2011},
author = {Marín, D. 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},
}