Fig. 6
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Comparison between AD Leo DS and a typical solar DS during a CME. (a) AD Leo VISAD spectrum with 200 s and 10 MHz averaging with a saturated colour scale. (b) A solar radio spectrum from Wind/WAVES instrument showing the different burst types associated with a solar CME on Jan 4, 2004. Solar type-IV and type-III features can be identified in the AD Leo spectrum. Solar data credit: CDAW data centre.
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