The low-high-low trend of type III radio burst starting frequencies and solar flare hard X-rays

Reid, Hamish A. S., Nicole Vilmer, and Eduard P. Kontar, The low-high-low trend of type III radio burst starting frequencies and solar flare hard X-rays, A&A, 567, A85 (2014) (ADS)

The cartoon

(click on the image for a larger version)

Garish colors are the surest way to the Archivist's heart. On the creative side, this one takes a redder look at the familiar caixa preta. Here is another stressful 2D view of the magic of reconnection, in the context of CSHKP, with a common point of confusion. The upward and downward beams, in the full CSHKP cartoon (see the Temmer one for more clashing colors), propagate on closed field lines in 3D, and therefore cannot produce type III bursts without further unspecified jiggery-pokery.

Date: 2019 December 18