@conference{10272/9339,
year = {2013},
url = {http://hdl.handle.net/10272/9339},
abstract = {High-sensitivity CCD video cameras
have been commonly used for the study of the
activity of meteoroid streams. These provide useful
data for the determination, for instance, of radiant,
orbital and photometric parameters [1, 2, 3]. These
devices can also be used to record emission spectra of
meteoroids ablating in the Earth's atmosphere when
holographic diffraction gratings are employed [3].
The SPMN is currently performing a continuous
monitoring of meteor activity by means of 25 meteor
observing stations in Spain. One important goal of our
network is the study of the physico-chemical properties
of meteoroids from multiple station data. These
include radiant and orbital parameters, but also chemical
information obtained from the emission spectra
produced during the ablation of these particles of interplanetary
matter in the atmosphere. This continuous
monitoring can provide useful data to improve our
knowledge about meteoroid streams and meteoroids of
sporadic origin, and the mechanisms that deliver these
materials to the Earth. With this aim, we analyze here a
sporadic fireball recorded on December 28, 2011.},
title = {Orbit and lines identification in the emission spectrum of a sporadic fireball},
author = {Zamorano, J. and Madiedo Gil, José María and Trigo Rodríguez, Josep María and Izquierdo Gómez, Jaime and Ocaña Gónzalez, Francisco and Sánchez de Miguel, A.},
}