HR: 0830h
AN: SH21B-0119    [PDF]
TI: Comparisons Between Noise Storm Emissions and CME Events
AU: * Marque, C
EM: christophe.marque@nrl.navy.mil
AF: Universities Space Research Association, Naval Research Laboratory 4555 Overlook Av S.W., Washington, DC 20375 United States
AU: Vourlidas, A
EM: angelos.vourlidas@nrl.navy.mil
AF: Georges Mason University, Naval Research Laboratory 4555 Overlook Av S.W., Washington, DC 20375 United States
AB: In this poster, we present preliminary comparisons between noise storm emissions and CME occurrences as observed with the Nan\c cay Radioheliograph and the LASCO coronagraph on board SOHO. We looked for modifications of the noise storm parameters (flux) and possible appearances or disappearances temporarily associated with CME initiation and propagation in the low corona. On-disk EUV images have also been used to locate the area where the CMEs were originating from.
DE: 7513 Coronal mass ejections
DE: 7534 Radio emissions
SC: SPA - Solar and Heliospheric Physics [SH]
MN: 2003 Fall Meeting