Type II Shocks Characteristics: Comparison with associated CMEs and Flares
G. Pothitakis, E. Mitsakou, P. Preka-Papadema, X. Moussas, C., Caroubalos, C.E. Alissandrakis, A. Hillaris, P. Tsitsipis, A. Kontogeorgos,, J.-L. Bougeret, G. Dumas
TL;DR
This study analyzes metric Type II radio bursts recorded between 1998-2000, comparing their characteristics with associated CMEs and flares to understand their origins and properties.
Contribution
It provides a comparative analysis of Type II shocks associated with CMEs and flares using observational data from ARTEMIS-IV.
Findings
Type II shocks show distinct characteristics depending on their association with CMEs or flares.
The study identifies differences in shock properties based on their origin.
Results enhance understanding of shock formation mechanisms in solar activity.
Abstract
A number of metric (100-650 MHz) typeII bursts was recorded by the ARTEMIS-IV radiospectrograph in the 1998-2000 period; the sample includes both CME driven shocks and shocks originating from flare blasts. We study their characteristics in comparison with characteristics of associated CMEs and flares.
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