Abstract
The solar coronal mass ejection observed on November 3, 2010 is analyzed using AIA/SDO data (images in the 193 and 211 Å channels) and white-corona images obtained with the SOHO LASCO C2 and C3 coronographs. We have succeeded in revealing both piston and blast-wave shocks attributed to the formation and propagation of a coronal mass ejection. Both of these types of shocks could be responsible for type II radio bursts propagating in front of each shock.
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Original Russian Text © V.G. Eselevich, M.V. Eselevich, I.V. Zimovets, 2013, published in Astronomicheskii Zhurnal, 2013, Vol. 90, No. 2, pp. 166–176.
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Eselevich, V.G., Eselevich, M.V. & Zimovets, I.V. Blast-wave and piston shocks connected with the formation and propagation of a coronal mass ejection. Astron. Rep. 57, 142–151 (2013). https://doi.org/10.1134/S1063772913020042
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DOI: https://doi.org/10.1134/S1063772913020042