G. Pothitakis, E. Mitsakou, P. Preka-Papadema, X. Moussas, C. Caroubalos, C. E. Alissandrakis, A. Hillaris, P. Tsitsipis, A. Kontogeorgos, J. -L. Bougeret, G. Dumas
Published 2010-09-22Version 1
A number of metric (100-650 MHz) typeII bursts was recorded by the ARTEMIS-IV radiospectrograph in the 1998-2000 period; the sample includes both CME driven shocks and shocks originating from flare blasts. We study their characteristics in comparison with characteristics of associated CMEs and flares.
Comments: Recent Advances in Astronomy and Astrophysics: 7th International Conference of the Hellenic Astronomical Society. AIP Conference Proceedings, Volume 848, pp. 238-242 (2006)
Journal: 2006AIPC..848..238P
Improved magnetogram calibration of SMFT and its comparison with the HMI
SEP acceleration in CME driven shocks using a hybrid code
Spatial & Temporal Characteristics of Ha flares during the period 1975-2002 (comparison with SXR flares)
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