Emission spectrum and orbital elements of two Quadrantid fireballs

Physics

Scientific paper

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Scientific paper

The activity of the Quadrantid meteor stream in 2011 has been monitored in the framework of the SPanish Meteor Network (SPMN). For this purpose, an array of high-sensitivity CCD video devices endowed with holographic diffraction gratings has been employed. Despite unfavorable weather conditions, we could image several bolides and their corresponding emission spectrum during the maximum activity period of this shower. We analyze here two of these Quadrantid fireballs.

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