Type II and IV radio bursts in the active period October-November 2003

TL;DR

This paper analyzes Type II and IV solar radio bursts observed in October-November 2003, highlighting their fine structures and association with solar flares and CMEs, using data from the ARTEMIS IV spectrograph.

Contribution

It provides detailed analysis of radio burst fine structures during a specific active period, linking them to solar flare and CME characteristics.

Findings

Rich fine structures observed in radio bursts

Association between burst features and solar flares/CMEs

Data from ARTEMIS IV enhances understanding of solar radio phenomena

Abstract

In this report we present the Type II and IV radio bursts observed and analyzed by the radio spectrograph ARTEMIS IV1, in the 650-20MHz frequency range, during the active period October-November 2003. These bursts exhibit very rich fine structures such fibers, pulsations and zebra patterns which is associated with certain characteristics of the associated solar flares and CMEs.