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Fine Structures of Solar Radio Type III Bursts and Their Possible Relationship with Coronal Density Turbulence

  • Authors: Xingyao Chen, Eduard P. Kontar, Sijie Yu, Yihua Yan, Jing Huang, and Baolin Tan

2018 The Astrophysical Journal 856 73.

  • Provider: AAS Journals

Caption: Figure 2.

(a) A composite of AIA images: 94 Å (red), 171 Å (green), and 193 Å (blue) highlighting the active regions (most of the red background). A 32.25 MHz LOFAR source at 11:56:56 UT is overlaid. (b) A composite image of AIA at the same time as (a), but using a different color table. The triangle symbols indicate the centroids of the fundamental LOFAR source at the frequencies and times corresponding to the green asterisks in Figure 3(a).

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