RT Conference Proceedings
T1 Recent developments in meteor spectroscopy in the framework of the S.M.A.R.T. proyect
A1 Madiedo Gil, José María
AB Meteor emission spectra provide aninsight into the chemical nature of meteoroids ablatingin the atmosphere, but also useful information aboutthe mechanisms that control this ablation process [1, 2,3, 4]. For this reason, an array of spectrographs hasbeen deployed at several meteor observing stationsoperated by the University of Huelva, in Spain. Thesestations work in the framework of the SPanish MeteorNetwork (SPMN). The first of these devices, whichwere based on low-lux CCD video cameras endowedwith holographic diffraction gratings, started operationin 2006 at the station in Sevilla and also at the CerroNegro mobile station [5]. Later on, slow-scan CCDspectrographs were also employed at both locations.Nowadays, these spectral cameras operate in a fullyautonomous way at 7 meteor stations in the frameworkof the SMART project, which is the acronym for Spectroscopyof Meteoroids in the Atmosphere by means ofRobotic Technologies. Favorable weather conditionsin Spain play a key role in the successful developmentof this systematic spectroscopic campaign. A descriptionof the main developments performed during 2013is given here.
YR 2014
FD 2014
LK http://hdl.handle.net/10272/9369
UL http://hdl.handle.net/10272/9369
LA eng
NO Madiedo Gil, J.M.: "Recent developments in meteor spectroscopy in the framework of the S.M.A.R.T. proyect". En: 45th Lunar and Planetary Science Conference (The Woolands, Texas, march 17-21, 2014)
DS Repositorio Institucional de la Universidad de Huelva
RD 30 may 2026