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Observations of the Quadrantid meteor shower from 2008 to 2012: orbits and emission spectra

机译:2008年至2012年Quadrantid流星雨的观测:轨道   和发射光谱

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摘要

The activity of the Quadrantids in January during several years (2008, 2010,2011 and 2012) has been investigated in the framework of the SPanish MeteorNetwork (SPMN). For this purpose, an array of high-sensitivity CCD videodevices and CCD all-sky cameras have been used to obtain multi-stationobservations of these meteors. These allowed us to obtain precise radiant andorbital information about this meteoroid stream. This paper presents a largeset of orbital data (namely, 85 orbits) of Quadrantid meteoroids. Most meteorsproduced by these particles were recorded during the activity peak of thisshower. Besides, we discuss four Quadrantid emission spectra. The tensilestrength of Quadrantid meteoroids has been also obtained.
机译:在SPanish MeteorNetwork(SPMN)的框架下,对象限在几年中(2008、2010、2011和2012年)的活动进行了调查。为此,已经使用了一系列高灵敏度CCD视频设备和CCD全天候摄像机来获取这些流星的多站观测。这些使我们能够获得有关该流星体流的精确辐射轨道信息。本文介绍了象限流星体的大量轨道数据(即85轨道)。由这些粒子产生的大多数流星记录在该淋浴的活动高峰期。此外,我们讨论了四个象限发射光谱。还获得了象限类星体的抗张强度。

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