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- W1676563525 abstract "We use dynamic spectra that display the observed radio intensity as a function of inverse frequency and time for tracking CME associated radio emissions through the interplanetary medium. The analyses of these radio emissions directly reveal the dynamics of the CME-driven shock as well as the nature of the radiation mechanism. For the two examples illustrated, we deduce that the type II radio emissions were generated primarily at the harmonic of the plasma frequency and in the upstream region of the CME-driven shock. For the two events, which have very different speeds, we found no evidence for significant deceleration of the CME-driven shock as it propagated through the interplanetary medium." @default.
- W1676563525 created "2016-06-24" @default.
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- W1676563525 date "1999-01-01" @default.
- W1676563525 modified "2023-10-14" @default.
- W1676563525 title "Remote radio tracking of CMEs in the solar corona and interplanetary medium" @default.
- W1676563525 doi "https://doi.org/10.1063/1.58709" @default.
- W1676563525 hasPublicationYear "1999" @default.
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