Energy Build-up and Release Mechanisms in Solar and Auroral Flares

Obayashi, T., Energy Build-up and Release Mechanisms in Solar and Auroral Flares, Sol. Phys., 40, 217-226 (1975) (ADS)

The cartoon

(click on the image for a larger version)

A prescient cartoon in a field (aurora/solar-flare analogy) that comes and goes with time (see Akasofu for another early one, and Martens-Kuin for some further physics). Has anybody learned anything further from this kind of exercise since this paper was written? At a rough guess 90% (or more) of all solar physicists could not define "Cowling conductivity," and indeed many of them happily ignore the mere existence of current carriers completely. This is of course not so surprising in view of the distressing lack of in-situ coronal plasma measurements, but there you are. The point is that magnetospheric physics is dominated by efforts to understand the behavior of currents and the detailed velocity distribution functions of the relevant particles that carry the electrical current, which varies widely by phenomenon. So any solar analogy will have to make all this stuff up somehow.

      In any case the author of this cartoon clearly shows the strong chromospheric perpendicular currents driven by the "collapse" of the emerged flux. The only wrinkle that could be added now might be the constraint on vertical current a la Melrose.

Date: 2007 April 21

Update: 2019 November 27