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Identification of infrasound produced by sprites during the Sprite2003 campaign

机译:识别Sprite2003活动期间精灵产生的次声

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摘要

During the summer of 2003, complementary measurements were taken in Europe during the Sprite2003 campaign to study sprites and associated processes. On July 21, 28 sprites observed by light-sensitive optical cameras located at the Observatoire du Pic du Midi in the Pyrenees mountains were found to correlate with chirp-like signals of several tenth to few minutes duration, measured by an infrasound station at Flers about 400 km from the thunderstorm. The sprite activity identified by the infrasound signature continued past sunrise into the daytime when optical systems cannot be used, documenting the occurrence of daytime sprites. Using an acoustic wave propagation model, the observed propagation delays, frequency dispersion, and duration of the infrasound bursts are found to be consistent with source altitudes at 60 - 80 km with horizontal dimensions equal to the optical width of the sprites. The chirp-like dispersion is a result of the propagation properties in the earth-thermosphere waveguide.
机译:在2003年夏季,Sprite2003运动期间在欧洲进行了补充测量,以研究Sprite及其相关过程。在7月21日,发现位于比利牛斯山脉比丘迪米迪天文台的光敏光学相机观测到的28个子星与持续了十分之几到几分钟的类似chi的信号有关,这是由Flers的次声台站测得的。距雷暴400公里。次声签名所标识的子画面活动一直持续到日出,直到白天无法使用光学系统,记录了白天子画面的发生。使用声波传播模型,发现观察到的传播延迟,频率色散和次声爆发的持续时间与60-80 km处的源高度(水平尺寸等于子图形的光学宽度)一致。线性调频色散是地球-地球大气波导中传播特性的结果。

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