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- W3139712487 abstract "We present an analysis of the dynamical evolution of interplanetary coronal mass ejections (ICMEs) and its associated Type II bursts.By using an analytical model developed to explain the ICME dynamics, we compute the speed, position and time of the ICME leading edge, in each point of the interplanetary space between the Sun and Earth. As inputs, the analytical model requires the initial (close to the Sun) and final (at one astronomical unit) ICME speeds, and iteratively computes the best parameters (CME mass and expansion rate, solar wind density, and drag coefficient) to fit both speeds.With this information, and assuming that the source of the type IIradio emission is at the nose of the ICME driven shock, we are able to predict the spectral behavior of the ICME-shock associated type II bursts.In this work, we present the model and its application to a set of ICMMEs which have an associated type II burst." @default.
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- W3139712487 date "2009-08-01" @default.
- W3139712487 modified "2023-09-23" @default.
- W3139712487 title "Interplanetary Evolution of Coronal Mass Ejections and Type II bursts" @default.
- W3139712487 hasPublicationYear "2009" @default.
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