Interchange Slip-Running Reconnection and Sweeping SEP Beams

Masson, S., G. Aulanier, E. Pariat, and K. L. Klein, Interchange Slip-Running Reconnection and Sweeping SEP Beams, Sol. Phys., 276, 199-217 (2012) (ADS)

The cartoon

(click on the image for a larger version)

This cartoon bravely attacks one of the outstanding problems of heliospheric physics, namely how the solar energetic particles spread out into a large solid angle within the solar wind. By a remarkable alphabetical coincidence, this is the same problem tackled in the adjacent Martinell cartoon but with greater artistic panache. This "escape" problem for SEPs has always seemed especially intractable for the type-III-burst electrons, at least as conventional wisdom understands them physically. These are identifiable with highly collimated soft X-ray jets, and one also can infer a tight beam structure directly and indirectly from the radio data. So, how does a point in space and time map onto a volume (or at least, onto an area)?

      The authors have "rounded up the usual suspect," to paraphrase Claude Rains: in this case, magnetic reconnection. This old and ill-understood concept is dressed up here with two adjectives: "slip-running" and "interchange", but it seems to be the same unknown microphysics as before. The problem has always been that a current sheet is basically a sheet, i.e. a a 2D manifold, whereas the solar wind is 3D. The authors discuss this in terms of the "spine" field line, which is 1D. So the Archivist is perplexed geometrically, seeking a space-filling (3D) population of SEPs and finding the wrong dimensionality in the proposed source.

Date: 2011 October 12

Update: 2019 November 26