dc.contributor.author | Alonso Azcárate, Jacinto | |
dc.contributor.author | Madiedo Gil, José María | |
dc.contributor.author | Trigo Rodríguez, Josep María | |
dc.contributor.author | Zamorano, J. | |
dc.contributor.author | Izquierdo Gómez, Jaime | |
dc.contributor.author | Ocaña Gónzalez, Francisco | |
dc.contributor.author | Sánchez de Miguel, A. | |
dc.contributor.author | Lacruz, J. | |
dc.contributor.author | Toscano, F. M. | |
dc.date.accessioned | 2014-11-18T12:49:59Z | |
dc.date.available | 2014-11-18T12:49:59Z | |
dc.date.issued | 2012 | |
dc.identifier.citation | Alonso Azcárate, Jacinto ; Madiedo Gil, José María ; Trigo Rodríguez, J.M., Zamorano, J., Izquierdo Gómez, J., Ocaña Gónzalez, F., Sánchez de Miguel, A., Lacruz, J., Toscano, F.M.: "Orbit and radiant of sporadic fireball imaged by the Spanish meteor network". En: 43rd Lunar and Planetary Science Conference ( (The Woolands, Texas, march 19-23, 2012) | |
dc.identifier.uri | http://hdl.handle.net/10272/9340 | |
dc.description.abstract | The development of a network of
meteor observing stations allows for a continuous
monitoring of meteor phenomena. One of the main
goals of the SPanish Meteor Network (SPMN) is the
analysis of the physico-chemical properties of meteoroids
from multiple station data. This provides useful
data to improve our knowledge about meteoroid
streams and meteoroids of sporadic origin, so that we
can reach a better understanding of the mechanisms
that deliver these materials to the Earth. In fact, the
orbits of large sporadic meteoroids are an important
source of impact hazard on the surfaces of artificial
satellites. We have started a continuous monitoring
program in order to get very reliable orbital data of
such a stochastic source to be able to improve models
of the meteoroid flux in the near-Earth environment
[1].
We currently operate 29 meteor observing stations
in Spain. Most of them employ high-sensitivity CCD
video devices, although low-scan all-sky CCD cameras
are also used. In this context, we have imaged on April
17, 2011 a four-station sporadic fireball with an absolute
magnitude of about -7±1. The analysis of this bolide
is presented here. | en_US |
dc.language.iso | eng | en_US |
dc.rights | Atribución-NoComercial-SinDerivadas 3.0 España | * |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/3.0/es/ | * |
dc.title | Orbit and radiant of sporadic fireball imaged by the Spanish meteor network | en_US |
dc.type | info:eu-repo/semantics/conferenceObject | en_US |
dc.rights.accessRights | info:eu-repo/semantics/openAccess | en_US |