First imaging spectroscopy observations of solar drift pair bursts

A. A. Kuznetsov; E. P. Kontar

doi:10.1051/0004-6361/201936447

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Volume 631 (November 2019)

A&A, 631 (2019) L7

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Fig. 6.

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Centroid locations of the emission sources of three selected emission features (same as in Figs. 3–5) overplotted on the SDO AIA 211 Å image. Contours of the radio intensity maps (corresponding to the frequency of 38 MHz) at half-maximum level are also shown.

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