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Simultaneous optical and radar observations of meteor head-echoes utilizing SAAMER

机译:利用SAAMER同时进行流星回波的光学和雷达观测

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摘要

We present simultaneous optical and radar observations of meteors observed with the Southern Argentine Agile MEteor Radar (SAAMER). Although such observations were performed in the past using High Power and Large Aperture radars, the focus here is on meteors that produced head echoes that can be detected by a significantly less sensitive but more accessible radar system. An observational campaign was conducted in August of 2011, where an optical imager was operated near the radar site in Rio Grande, Tierra del Fuego, Argentina. Six head echo events out of 150 total detections were identified where simultaneous optical meteors could also be clearly seen within the main radar beam. The location of the meteors derived from the radar interferometry agreed very well with the optical location, verifying the accuracy of the radar interferometry technique. The meteor speeds and origin directions calculated from the radar data were accurate compared with the optics for the 2 meteors that had radar signal-to-noise ratios above 2.5. The optical meteors that produced the head echoes had horizontal velocities in the range of 29-91 km/s. These comparisons with optical observations improve the accuracy of the radar detection and analysis techniques, such that, when applied over longer periods of time, will improve the statistics of southern hemisphere meteor observations. Mass estimates were derived using both the optical and radar data and the resulting masses agreed well with each other. All were within an order of magnitude and in most cases, the agreement was within a factor of two. (C) 2015 Elsevier Ltd. All rights reserved.
机译:我们介绍了同时利用阿根廷南部敏捷流星雷达(SAAMER)观测到的流星的光学和雷达观测。尽管过去使用大功率和大孔径雷达进行了此类观测,但这里的重点是流星产生的头部回声,而这种回声可以通过灵敏度明显较低但更易于访问的雷达系统检测到。 2011年8月进行了一场观察运动,其中一台光学成像仪在阿根廷火地岛里奥格兰德的雷达场附近操作。在150次总探测中,有6次头部回声事件被识别出来,同时在主雷达波束内也可以清晰地看到同时的流星。由雷达干涉测量法得出的流星的位置与光学位置非常吻合,验证了雷达干涉测量技术的准确性。与雷达信噪比高于2.5的2颗流星的光学器件相比,根据雷达数据计算出的流星速度和原点方向是准确的。产生头部回波的光学流星的水平速度范围为29-91 km / s。这些与光学观测的比较提高了雷达探测和分析技术的准确性,因此,如果长时间应用,将改善南半球流星观测的统计数据。使用光学和雷达数据得出质量估计,得到的质量彼此一致。所有这些都在一个数量级之内,并且在大多数情况下,一致性在两个因数之内。 (C)2015 Elsevier Ltd.保留所有权利。

著录项

  • 来源
    《Planetary and space science》 |2015年第12期|95-101|共7页
  • 作者单位

    Univ Maryland, College Pk, MD 20742 USA|NASA, Goddard Space Flight Ctr, Greenbelt, MD USA;

    NASA, Goddard Space Flight Ctr, Greenbelt, MD USA;

    NASA, Goddard Space Flight Ctr, Greenbelt, MD USA;

    Estn Astron Rio Grande, Rio Grande, Tierra Del Fueg, Argentina;

    Natl Univ La Plata, Dept Ciencias Astron & Geofis, La Plata, Buenos Aires, Argentina;

    Natl Univ La Plata, Dept Ciencias Astron & Geofis, La Plata, Buenos Aires, Argentina;

  • 收录信息
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    Meteor; Optical; Head echo; Meteor mass;

    机译:流星;光学;头回波;流星质量;

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