Sun-related variability in the light curves of compact radio sources - A new view on extreme scattering events

Open Access

Fig. 5.

GBI and UMRAO light curves of 0528+134. Brown lines indicate the ESEs identified by Lazio et al. (2001a), while turquoise ones show three more simultaneous multi-frequency dips recognisable in the data. In the small box we show the 1988.9 event, a rare example of a complex ESE shape observable at 2 GHz.

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