Development Of Coronal Mass Ejections : Radio Shock Signatures

Details Development Of Coronal Mass Ejections : Radio Shock Signatures Development Of Coronal Mass Ejections : Radio Shock Signatures

Oct 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999esasp.446..473m&link_type=abstract

8th SOHO Workshop: Plasma Dynamics and Diagnostics in the Solar Transition Region and Corona. Proceedings of the Conference hel

Astronomy and Astrophysics

Astrophysics

Scientific paper

This study presents joint observations of Coronal Mass Ejections from the EIT telescope and LASCO coronagraphs on SOHO and from the Nan ay Radioheliograph. The contribution of radio observations to the present knowledge of origin and development of CMEs will be reviewed. In particular, this study will focuss on the following points : - The radio detection in the corona of the leading edge of CMEs and the association with shocks ; - The identification of successive sequences leading to the full development of CMEs and the timing of these sequences. The radio detection of coronal waves- The radio counterpart seen in projection over the solar disk of halo CME events.

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