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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Toward the azimuthal characteristics of ionospheric and seismic effects of 'Chelyabinsk'meteorite fall according to the data fromcoherent radar, GPS, and seismic networks
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Toward the azimuthal characteristics of ionospheric and seismic effects of 'Chelyabinsk'meteorite fall according to the data fromcoherent radar, GPS, and seismic networks

机译:根据相干雷达,GPS和地震网络的数据,对“车里雅宾斯克”陨石的电离层方位特征和地震效应下降

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We present the results of a study of the azimuthal characteristics of ionospheric and seismic effects of the meteorite 'Chelyabinsk,' based on the data from the network of GPS receivers, coherent decameter radar EKB, and network of seismic stations, located near the meteorite fall trajectory. It is shown that 6–14 min after the bolide explosion, GPS network observed the cone-shaped wavefront of traveling ionospheric disturbances (TIDs) that is interpreted as a ballistic acoustic wave. The typical TIDs propagation velocity were observed 661 ± 256 m/s, which corresponds to the expected acoustic wave speed for 240 km height. Fourteen minutes after the bolide explosion, at distances of 200 km, we observed the emergence and propagation of a TID with annular wavefront that is interpreted as gravitational mode of internal atmospheric waves. The propagation velocity of this TID was 337 ± 89 m/s which corresponds to the propagation velocity of these waves in similar situations. At EKB radar, we observed TIDs in the sector of azimuthal angles close to the perpendicular to the meteorite trajectory. The observed TID velocity (400 m/s) and azimuthal properties correlate well with the model of ballistic wave propagating at 120–140 km altitude. It is shown that the azimuthal distribution of the amplitude of vertical seismic oscillations with periods 3–60 s can be described qualitatively by the model of vertical strike-slip rupture, propagating at 1 km/s along the meteorite fall trajectory to distance of about 40 km. These parameters correspond to the direction and velocity of propagation of the ballistic wave peak by the ground. It is shown that the model of ballistic wave caused by supersonic motion and burning of the meteorite in the upper atmosphere can satisfactorily explain the various azimuthal ionospheric effects, observed by the coherent decameter radar EKB, GPS receivers network, and the azimuthal characteristics of seismic waves at large distances.
机译:我们根据来自GPS接收器网络,相干十进制雷达EKB和位于陨石坠落附近的地震台网的数据,对陨石“车里雅宾斯克”的电离层方位特性和地震效应进行研究,得出结果。弹道。结果表明,在硼化物爆炸后6–14分钟,GPS网络观测到了行进的电离层扰动(TID)的锥形波阵面,该波阵面被解释为弹道声波。观察到的典型TID传播速度为661±256 m / s,对应于240 km高度的预期声波速度。爆炸发生后14分钟,在200 km的距离上,我们观察到TID的出现和传播,该TID具有环形波前,这被解释为内部大气波的重力模式。该TID的传播速度为337±89 m / s,对应于类似情况下这些波的传播速度。在EKB雷达上,我们在接近陨石轨迹的垂直线的方位角扇区中观测到TID。观测到的TID速度(400 m / s)和方位角特性与在120–140 km高度传播的弹道波模型很好地相关。结果表明,垂直地震振荡振幅的方位角分布可以用垂直走滑破裂模型定性地描述,该模型沿陨石坠落轨迹以1 km / s的速度传播到距离大约40的距离,定性描述公里这些参数对应于弹道波峰被地面传播的方向和速度。结果表明,由相干十进制雷达EKB,GPS接收器网络和地震波的方位角特征所观测到的,由超音速运动和陨石在高层大气中燃烧引起的弹道波模型可以令人满意地解释各种方位电离层效应。在远处。

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