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arXiv · 1009.4310

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
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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.

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K. Bouratzis, P. Preka-Papadema, A. Hillaris, X. Moussas, C. Caroubalos, V. Petoussis, P. Tsitsipis, A. Kontogeorgos. 2010-09-22. Radio Bursts in the Active Period January 2005. https://doi.org/10.1063/1.2347980

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