Coronal Mass Ejections and their Associated Radio Emissions

Details Coronal Mass Ejections and their Associated Radio Emissions Coronal Mass Ejections and their Associated Radio Emissions

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agusmsh24a..02b&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SH24A-02

Physics

Plasma Physics

7500 Solar Physics, Astrophysics, And Astronomy, 7513 Coronal Mass Ejections (2101), 7534 Radio Emissions, 7800 Space Plasma Physics

Scientific paper

Coronal mass ejections (CMEs) are important drivers of processes in the interplanetary medium and the near- Earth environment, including shocks, CMEs, and geomagnetic disturbances. Radio observations of CMEs and associated phenomena offer a number of unique diagnostics of CMEs and their environment in the nascent stages of their development. These include thermal free-free radiation, nonthermal synchrotron radiation, and plasma radiation. These emissions can be used to constrain the plasma properties of CMEs - including the plasma density and magnetic field - as they propagate outward from the Sun. Under certain conditions, they can probe the response of the corona to the CME. Some recent and suggestive observations are presented of radio emission from CMEs, as well as of associated radio bursts.

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