Reducing heliospheric magnetic flux from coronal mass ejections without disconnection

Crooker, N. U., J. T. Gosling, and S. W. Kahler, Reducing heliospheric magnetic flux from coronal mass ejections without disconnection, Journal of Geophysical Research (Space Physics), 107, 1028 (2002) (ADS)

The cartoon

(click on the image for a larger version)

The is the cartoon defining "interchange reconnection," a concept rewarmed for the heliospheric community from older solar ideas (many in this Archive). The paper introducing this idea attempts to explain what the Archivist thinks of as "Gold's paradox," described also in the much earlier Gold cartoon here. It is the quandary associated with the incremental increase of heliospheric open field as a result of CME action. This paradox still seems interesting, and this paper does little in fact to explain it. Part of the problem is in nomenclature, and of course introducing the word "interchange" immediately causes superficial confusion with the concept of the "interchange instability." The solar and heliospheric communities do not mean the same thing by "open field line," and of course any physicist trusting to the reality of field lines in the first place is likely to be heading for confusion. For example, one could argue that if a flux tube contains a wind-type flow (super-Alfvénic) it is open; on the other hand non-thermal tail particles could in principle leave the Sun and then return to it basically within the same flux tube - thus one could say that the field is closed.

      All this may become clearer if you also ponder the Crooker-Pagel cartoon.

Date: 2007 March 25

Update: 2019 February 12