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Fig. 6.


a: superposition of noise storm contours at 432 MHz and 237 MHz onto an EIT image at 09:50 UT on July 14, 2000. b: superposition of the sources on the photospheric magnetogram (MDI) and coronal field lines inferred using the PFSS model by Schrijver & De Rosa (2003). The magnetic configuration associated with the streamer regions are indicated by red arrows. The streamer associated with NS1 was examined by Török et al. (2018). c: superposition of the radio sources on an MDI magnetogram.

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