Comment – on ‘Analysis of Petschek-Type Reconnection in Non-Uniform Field and Flow Geometries’, by Michael T. Kiendl,Vladimir S. Semenov,Igor V. Kubyshkin,Helfried K. Biernat,Richard P. Rijnbeek,and Bruno P. Besser

Space Science Reviews -     

CME dynamics using coronagraph and interplanetary ejecta data

In this work, we present a study of the coronal mass ejection (CME) dynamics using LASCO coronagraph observations combined with in-situ ACE plasma and magnetic field data, covering a continuous period of time from January 1997 to April 2001, complemented by few extreme events observed in 2001 and 2003. We show, for the first time, that the CME expansion speed correlates very well with the travel time to 1 AU of the interplanetary ejecta (or ICMEs) associated with the CMEs, as well as with their preceding shocks. The events analyzed in this work are a subset of the events studied in Schwenn et al. (2005), from which only the CMEs associated with interplanetary ejecta (ICMEs) were selected. Three models to predict CME travel time to Earth, two proposed by Gopalswamy et al. (2001) and one by Schwenn et al. (2005), were used to characterize the dynamical behavior of this set of events. Extreme events occurred in 2001 and 2003 were used to test the prediction capability of the models regarding CMEs with very high LASCO C3 speeds.     

一种计算转子不平衡响应的新方法

建立了以状态方程和转移矩阵为基础的分析方法，以分析复杂转子的不平衡响应。在不必事先确定转子系统固有振型及自振频率的情况下，利用此方法可直接求得转子振动响应的精确解。该方法与传递矩阵法相结合，可容易地求解复杂转子系统的不平衡响应问题。算例分析表明，该方法简捷有效