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arXiv 2608.17589astro-ph.EPphysics.space-ph

PANSY流星头回波轨道星表:南极雷达对南天天流星体流的连续观测

The PANSY Meteor Head-echo Orbit Catalogue: Continuous Antarctic Radar Observations of Southern Meteoroid Streams

Juha Vierinen, Jorge L. Chau, Koji Nishimura, Taishi Hashimoto, Nico Pfeffer, Daniel Kastinen, Devin R. Huyghebaert, Johan Kero, Masaki Tsutsumi, Kaoru Sato

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中文总结 AI 辅助

研究发布基于南极PANSY雷达的首个流星头回波轨道星表,含200万颗流星等数据,发现新流星雨候选体,助力南半球近地流星体群研究。

中文摘要 AI 辅助

高功率大口径雷达的流星头回波可为亚毫米半径范围内的单个微流星体提供脉冲分辨的位置和速度,这些微流星体对地球的质量流入贡献显著。我们公布了首个基于南极昭和中层-平流层-对流层/非相干散射雷达(PANSY)的流星头回波轨道星表,该星表包含200万颗流星和5000万次脉冲分辨测量。观测到的辐射点分布包含日心、反日心、南环带和顶源,提供了前所未有的南天 ecliptic 纬度的头回波覆盖。初始探测高度分布呈双带结构,两条带均随流星速度升高而高度增加,且呈现不同的辐射点分布,这与流星体尺寸差异和 differential ablation( differential ablation: differential ablation 为专有名词,保留原名)的混合效应一致。动态质量估算表明,该巡天对初始半径约100微米的流星体敏感。作为星表初步探索的一部分,我们研究了夜间摩羯座α流星雨(CAP)和扩展的白天摩羯座-人马座流星雨(DCS)辐射点,它们在相反节点的相似活动时长符合其属于CAP-169P/NEAT复合体的成员身份。辐射点分布暗示存在一个新的流星雨候选体,其峰值流量接近太阳经度110°,平均日心 ecliptic 辐射点经度291.0°、纬度-48.2°,地心速度48.7 km s⁻¹。在星表生成过程中,事件级原始电压数据被临时保留以支持数据分析的改进。本次首次星表发布覆盖2025年1月26日至2026年7月26日,将有助于进一步研究南半球近地流星体群。

英文摘要

Meteor head echoes from high-power, large-aperture radars provide pulse-resolved positions and velocities for individual micrometeoroids in a submillimeter-radius range that contribute significantly to the mass influx to Earth. We present the first meteor head-echo orbit catalogue from the Antarctic Syowa Mesosphere--Stratosphere--Troposphere/Incoherent Scatter radar (PANSY). The catalogue contains two million meteors and 50 million pulse-resolved measurements. The observed radiant distribution contains the helion, antihelion, south toroidal and apex sources, and provides unprecedented head-echo coverage of southern ecliptic latitudes. The initial detection-height distribution is found to be double-banded, with both bands increasing in height with meteor speed and exhibiting distinct radiant distributions, consistent with a mixture of meteoroid-size differences and differential ablation. Estimation of dynamic mass indicates that the survey is sensitive to initial radii of approximately 100 micrometers. As part of an initial exploration of the catalogue, we investigate the nighttime alpha Capricornids (CAP) and the extended Daytime Capricornids-Sagittariids (DCS) radiant. Their similar activity durations at opposite nodes are consistent with membership in the CAP--169P/NEAT complex. The radiant distribution suggests a new meteor shower candidate, with peak flux near solar longitude 110 degrees, mean Sun-centered ecliptic radiant longitude 291.0 degrees, latitude -48.2 degrees, and geocentric speed 48.7 km s^{-1}. During catalogue production, event-level raw voltage cuts are retained temporarily to support improvements in data analysis. This first catalogue release, covering 2025 January 26 to 2026 July 26, will be useful for further studies of the southern-hemisphere Earth-crossing meteoroid population.

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