Type III Radio Bursts and the Structure of the Inner Heliosphere

Details Type III Radio Bursts and the Structure of the Inner Heliosphere Type III Radio Bursts and the Structure of the Inner Heliosphere

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003agufmsh42e..05r&link_type=abstract

American Geophysical Union, Fall Meeting 2003, abstract #SH42E-05

Physics

2139 Interplanetary Shocks, 2194 Instruments And Techniques, 7509 Corona, 7513 Coronal Mass Ejections, 7534 Radio Emissions

Scientific paper

Type III solar radio bursts provide important information on the origin, acceleration, and propagation of particles associated with solar flares and coronal shocks. Since these radio emissions are generated by the plasma emission mechanism, observations of these solar radio transients also provide remote sensing of the plasma conditions in the corona and of the magnetic and plasma structure of the inner heliosphere. In this talk I will review the progress of type III research from their discovery in the late 40s to the most recent advances from low-frequency spacecraft observations, primarily from ISEE-3, Wind and Ulysses.

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