Radio Bursts in the Active Period January 2005

K. Bouratzis; P. Preka-Papadema; A. Hillaris; X. Moussas; C. Caroubalos; V. Petoussis; P. Tsitsipis; A. Kontogeorgos

doi:10.1063/1.2347980

paper

Radio Bursts in the Active Period January 2005

arXiv:1009.4310 · doi:10.1063/1.2347980

Abstract

We present complex radio bursts recorded by the radiospectrograph ARTEMIS-IV in the active period of January 2005. The wide spectral coverage of this recorder, in the 650-20 MHz range, permits an analysis of the radio bursts from the base of the Solar Corona to 2 Solar Radii; it thus facilitates the association of radio activity with other types of solar energetic phenomena. Furthermore the ARTEMIS-IV1, high time resolution (1/100 sec) in the 450-270 MHz range, makes possible the detection and analysis of the fine structure which most of the major radio events exhibit.

arXiv commentRecent Advances in Astronomy and Astrophysics: 7th International Conference of the Hellenic Astronomical Society. AIP Conference Proceedings, Volume 848, pp. 213-217 (2006)