most citedA possible mechanism of energy dissipation in the front of a shock wave driven ahead of a coronal mass ejection

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astro-ph.SR2009★ 1 cited

A possible mechanism of energy dissipation in the front of a shock wave driven ahead of a coronal mass ejection

M. Eselevich, V. Eselevich

Mark 4 and LASCO C2, C3 coronagraph data analysis shows that, up to the distance 5 R from the center of the Sun, the thickness of a CME-generated shock front may be…