首页> 外文期刊>Annales Geophysicae >Speed evolution of fast CME/shocks with SOHO/LASCO, WIND/WAVES, IPS and in-situ WIND data: analysis of kilometric type-II emissions
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Speed evolution of fast CME/shocks with SOHO/LASCO, WIND/WAVES, IPS and in-situ WIND data: analysis of kilometric type-II emissions

机译:利用SOHO / LASCO,WIND / WAVES,IPS和原位WIND数据加快CME /电击的快速发展:II型公里排放量的分析

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Fast CME/shocks propagating in the interplanetary medium can generate kilometric Type II (km-TII) radio emissions at the local plasma frequency and/or its harmonic, so these radio emissions provide a means of remotely tracking CME/shocks. We apply a new analysis technique, using the frequency drift of km-TII spectrum obtained by the Thermal Noise Receiver (TNR) of the WIND/WAVES experiment, to infer, at some adequate intervals, the propagation speed of six CME/shocks. We combine these results with previously reported speeds from coronagraph white light and interplanetary scintillation observations, and in-situ measurements, to study the temporal speed evolution of the six events. The speed values obtained by the km-TII analysis are in a reasonable agreement with the speed measurements obtained by other techniques at different heliocentric distance ranges. The combination of all the speed measurements show a gradual deceleration of the CME/shocks as they propagate to 1 AU. This new technique can be useful in studying the evolution of fast CME/shocks when adequate intervals of km-TII emissions are available.
机译:在行星际介质中传播的快速CME /激波可以在本地等离子频率和/或其谐波下产生公里数的II型(km-TII)无线电辐射,因此这些无线电辐射提供了一种远程跟踪CME /激波的方法。我们应用一种新的分析技术,利用WIND / WAVES实验的热噪声接收器(TNR)获得的km-TII频谱的频率漂移,以一定的间隔推断六个CME /震波的传播速度。我们将这些结果与先前报道的日冕仪白光和行星际闪烁观测以及原位测量的速度相结合,以研究这六个事件的时间速度演变。 km-TII分析获得的速度值与其他技术在不同日心距范围内获得的速度测量值在合理范围内一致。所有速度测量值的组合显示CME /震荡传播到1 AU时逐渐减速。当有足够的km-TII排放间隔时,这项新技术可用于研究快速CME /电击的演变。

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