Author/Authors :
A. Hillaris، نويسنده , , V. Petousis، نويسنده , , E. Mitsakou، نويسنده , , Melina C. Vassiliou، نويسنده , , X. Moussas، نويسنده , , J. Polygiannakis، نويسنده , , P. Preka-Papadema، نويسنده , , C. Caroubalos، نويسنده , , C. Alissandrakis، نويسنده , , P. Tsitsipis، نويسنده , , A. Kontogeorgos، نويسنده , , J.-L. Bougeret، نويسنده , , G. Dumas، نويسنده ,
Abstract :
We analyse of a set of radio rich (accompanied by type IV or II bursts) solar flares and their association with SOHO/LASCO Coronal Mass Ejections in the period 1998–2000. The intensity, impulsiveness and energetics of these events are investigated. We find that, on the average, flares associated both with type IIs and CMEs are more impulsive and more energetic than flares associated with type IIs only (without CME reported), as well as flares accompanied by type IV continua but not type II shocks. From the last two classes, flares with type II bursts (without CMEs reported) are the shortest in duration and the most impulsive.
Keywords :
Sun: coronal mass ejections , Sun: X-rays , Sun: Activity , Sun: flares
