Shock location and CME 3-D reconstruction of a solar type II radio burst with LOFAR by P. Zucca et al.* – Community of European Solar Radio Astronomers
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![PDF] Shock Location and CME 3-D Reconstruction of a Solar Type II Radio Burst with LOFAR | Semantic Scholar](https://d3i71xaburhd42.cloudfront.net/7266700f2023e4da7506f35368f1bc4a62918f18/5-Figure5-1.png "PDF] Shock Location and CME 3-D Reconstruction of a Solar Type II Radio Burst with LOFAR | Semantic Scholar")
PDF] Shock Location and CME 3-D Reconstruction of a Solar Type II Radio Burst with LOFAR | Semantic Scholar
7. Snapshot map of the radio CME loops at 164 MHz. The background disk... | Download Scientific Diagram
a) Snapshot map of the radio CME at a frequency of 164 MHz at the... | Download Scientific Diagram
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Illustration of a coronal mass ejection (CME) emanating from the Sun. These events are powerful releases of solar charged particles (plasma) and magnetic field, travelling on the solar wind. When a CME
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