C. Caroubalos

TL;DR: The new solar radiospectrograph of the University of Athens operating at the Thermopylae Station since 1996 is presented, used either by itself to study the onset and evolution of solar radio bursts or in conjunction with other instruments including the Nançay Decametric Array and the WIND/WAVES RAD1 and RAD2 low frequencyreceivers to study associated interplanetary phenomena.

TL;DR: In this article, an almost com- plete frequency coverage of a shock-associated (SA) radio event and related phenomena observed on May 6, 1996 at 9:27 UT is presented.

TL;DR: In this article, the authors infer the potential source locations of the radio emission of the coronal mass ejection on the SDO Atmospheric Imaging Assembly (AIA) images, and show that the expansion of the CME ejecta is the source for both EUV and radio shock emissions.

TL;DR: In this article, the authors infer the potential source locations of the radio emission of the coronal mass ejection (CME) from the AIA images using a novel technique, which deduces a proxy of the EUV compression ratio from AIA imaging data and compares it with the compression ratio deduced from the band split of the Type II metric radio burst.

TL;DR: A catalogue of the type II and type IV solar radio bursts in the 110-687 MHz range, observed with the radio spectrograph ARTEMIS-IV operated by the University of Athens at Thermopylae, Greece from 1998-2000 is presented in this paper.