RT Conference Proceedings
T1 Orbit and lines identification in the emission spectrum of a sporadic fireball
A1 Zamorano, J.
A1 Madiedo Gil, José María
A1 Trigo Rodríguez, Josep María
A1 Izquierdo Gómez, Jaime
A1 Ocaña Gónzalez, Francisco
A1 Sánchez de Miguel, A.
AB High-sensitivity CCD video camerashave been commonly used for the study of theactivity of meteoroid streams. These provide usefuldata for the determination, for instance, of radiant,orbital and photometric parameters [1, 2, 3]. Thesedevices can also be used to record emission spectra ofmeteoroids ablating in the Earth's atmosphere whenholographic diffraction gratings are employed [3].The SPMN is currently performing a continuousmonitoring of meteor activity by means of 25 meteorobserving stations in Spain. One important goal of ournetwork is the study of the physico-chemical propertiesof meteoroids from multiple station data. Theseinclude radiant and orbital parameters, but also chemicalinformation obtained from the emission spectraproduced during the ablation of these particles of interplanetarymatter in the atmosphere. This continuousmonitoring can provide useful data to improve ourknowledge about meteoroid streams and meteoroids ofsporadic origin, and the mechanisms that deliver thesematerials to the Earth. With this aim, we analyze here asporadic fireball recorded on December 28, 2011.
YR 2013
FD 2013
LK http://hdl.handle.net/10272/9339
UL http://hdl.handle.net/10272/9339
LA eng
NO Zamorano, J., Madiedo Gil, J.M., Trigo Rodríguez, J.M., Izquierdo Gómez, J., Ocaña Gónzalez, F., Sánchez de Miguel, A.: "Orbit and lines identification in the emission spectrum of a sporadic fireball". En: 44th Lunar and Planetary Science Conference (The Woolands, Texas, march 18-22, 2013)
DS Repositorio Institucional de la Universidad de Huelva
RD 31 may 2026