The Alfvén-Wave Theory of Solar Flares

Piddington, J. H., The Alfvén-Wave Theory of Solar Flares, Sol. Phys., 38, 465-481 (1974) (ADS)

The cartoon

(click on the image for a larger version)

This cartoon assaults the eye, even in humble black and white! This is one of several cartoons in this important paper, which should really have catapulted Piddington into the CSHKP pantheon. This cartoon was just too imposing to ignore. The whorls show what Moore calls the "sheared core" field, which is held in place by an overlying toroidal field connecting the model sunspots. In this paper Piddington also continues his description of twisted flux-tube emergence. All in all Piddington seems to have created many of the concepts we regard as modern today - when one thinks of the innovations of Giovanelli as well, one has to be impressed by Australian inventiveness. And, for sheer visual impact, this cartoon rivals that of Longcope, which in fact has no visible shear!

      Here everything is attributed to Alfvén-wave transport, except for particle acceleration (tentatively assigned to magnetic reconnection, for want of any available microphysics). The description is in terms of upwards energy flows, however, whereas the Archivist thinks that some important energy transport must be downwards. But this idea has finally caught on.

Date: 2007 December 28

Update: 2019 November 27