Multi-spacecraft Observations of Type II Radio Emission

Details Multi-spacecraft Observations of Type II Radio Emission Multi-spacecraft Observations of Type II Radio Emission

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011agufmsh23c1976a&link_type=abstract

American Geophysical Union, Fall Meeting 2011, abstract #SH23C-1976

Astronomy and Astrophysics

Astrophysics

[7534] Solar Physics, Astrophysics, And Astronomy / Radio Emissions

Scientific paper

Interplanetary Type II radio burst radiation results from the excitation of plasma waves in the ambient medium by shock waves driven by coronal mass ejections (CMEs). These radio emissions provide a means of remotely tracking CME/shocks. The aim of this work is to present an analysis of some events of Type II radio bursts observed by Wind/WAVES and STEREO/SWAVES radio instruments. We focus our analysis on the spectral properties of the Type II emissions and the speed evolution of CME/shocks. Linking remote-sensing observations with in-situ measurements provides a useful tool to track CME/shocks that move outward from the Sun to 1 AU.

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