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.
@article{arxiv.1009.4310,
title = {Radio Bursts in the Active Period January 2005},
author = {K. Bouratzis and P. Preka-Papadema and A. Hillaris and X. Moussas and C. Caroubalos and V. Petoussis and P. Tsitsipis and A. Kontogeorgos},
journal= {arXiv preprint arXiv:1009.4310},
year = {2010}
}
Comments
Recent Advances in Astronomy and Astrophysics: 7th International Conference of the Hellenic Astronomical Society. AIP Conference Proceedings, Volume 848, pp. 213-217 (2006)