Zeuzzz
Banned
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- Dec 26, 2007
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Actually, its probably best I put this post here.
While the explanation is not strictly current disruption, it follows a similar approach, instead of using magetic field lines and flux transfer it considers the way that the currents and resulting dynamo's they produce can be a viable contendor to magnetic reconnection.
Instead of relying on the concept of magnetic reconnection, world authority on magnetosphric physics Syun-Ichi Akasofu and others, have recently shown in a publication in the IEEE transactions on plasma science, that it may be worthwhile to consider that the solar wind–magnetosphere dynamo generates two solenoidal currents in the magnetotail. The flux transfer can be understood in terms of an increase of the solenoidal currents caused by an increase of ε. Changes of the magnetic field configuration that are associated with the so-called “southward turning” of the IMF vector can be explained by an increase of the dynamo power ε.
Long Standing Unsolved Problems in Solar–Terrestrial Physics - Plasma Science, IEEE Transactions on, Dec. 2007
Much more plausable than MR in my opinion, as by focussing on electric field and current as primary quantities you can consider an analysis based on detailed particle dynamics, instead of the interaction of ambiguos field lines and MHD terms, that lead to many problems. He ellaborates on this model further later, but i'm restricted to small quote size on this forum, and people throw a fit when I post stuff not in quotes. I suspect that such electrical solutions like this are evident in most situations where MR is utilised, and can usually provide a much more detailed explanation of what is physically occuring than MR does. I am not saying that MR is completely redundant, it can be useful in working out flux transfer, but the question is whether MR is the final tool in understanding substorms. Although many MHD simulations have been successful in reproducing substorm-like features, they have not actually come up with a chain of processes that lead to a substorm onset, partly because the reconnection rate is arbitrarily set.
Really, reconnection cannot happen? Do you have any proof for that?
And please give us the description of current disruption re-organization of the magnetic field topology.
Don't forget that in the Earth's magnetotail we have a enormous amount of observations of magnetic field and plasma that all totally agree with the model of magnetic reconnection. I would love to see your explanation.
While the explanation is not strictly current disruption, it follows a similar approach, instead of using magetic field lines and flux transfer it considers the way that the currents and resulting dynamo's they produce can be a viable contendor to magnetic reconnection.
Instead of relying on the concept of magnetic reconnection, world authority on magnetosphric physics Syun-Ichi Akasofu and others, have recently shown in a publication in the IEEE transactions on plasma science, that it may be worthwhile to consider that the solar wind–magnetosphere dynamo generates two solenoidal currents in the magnetotail. The flux transfer can be understood in terms of an increase of the solenoidal currents caused by an increase of ε. Changes of the magnetic field configuration that are associated with the so-called “southward turning” of the IMF vector can be explained by an increase of the dynamo power ε.
Long Standing Unsolved Problems in Solar–Terrestrial Physics - Plasma Science, IEEE Transactions on, Dec. 2007
As ε increases, the two solenoidal currents increase in the magnetotail, and the resulting increase of the antiparallel flux can cause changes of the magnetic field configuration in both the dayside and the nightside. The changes are basically the same with those caused by the magnetic flux transfer to the nightside. An enhanced antiparallel field in the magnetotail stretches the dipolar field in the nightside. (Fig. 8).
As will be discussed in the next section, some substorms are triggered by a sudden “northward turning” of the IMF vector after the magnetosphere is primed [26]. As the ε is decreased, the intensity of themagnetotail field is decreased. It has been interpreted, however, that the decrease of the magnetotail field is a proof of magnetic reconnection [13]. This argument forgets the fact that the northward turning indicates a decrease of the solenoidal (cross-tail) current after an enhancement during the period of being primed. Our way of interpreting such phenomena can help in avoiding misinterpretation that the field decrease is caused by magnetic reconnection. This way of consideration, although not quantitative, does not require the knowledge of the reconnection rate, which is uncertain (making the quantitativeness of the MHD simulation somewhat doubtful). It is unfortunate that theorists are not interested in such a simple way of understanding magnetospheric phenomena. This will become more evident in the next section. Thus, this qualitative way may be more accurate than a quantitative misinterpretation based on magnetic reconnection.
[13] M. N. Caan, R. L.McPherron, and C. T. Russell, “Substorm and interplanetary magnetic field effects on the geomagnetic tail lobes,” J. Geophys. Res., vol. 80, pp. 191–194, Jan. 1975.
[26] L. R. Lyons, G. T. Blanchard, J. C. Samson, R. P. Lepping, T. Yamamoto, and T. Moretto, “Coordinated observations demonstrating external substorm triggering,” J. Geophys. Res., vol. 102, no. A12, pp. 27 039–27 051, Dec. 1, 1997.
Much more plausable than MR in my opinion, as by focussing on electric field and current as primary quantities you can consider an analysis based on detailed particle dynamics, instead of the interaction of ambiguos field lines and MHD terms, that lead to many problems. He ellaborates on this model further later, but i'm restricted to small quote size on this forum, and people throw a fit when I post stuff not in quotes. I suspect that such electrical solutions like this are evident in most situations where MR is utilised, and can usually provide a much more detailed explanation of what is physically occuring than MR does. I am not saying that MR is completely redundant, it can be useful in working out flux transfer, but the question is whether MR is the final tool in understanding substorms. Although many MHD simulations have been successful in reproducing substorm-like features, they have not actually come up with a chain of processes that lead to a substorm onset, partly because the reconnection rate is arbitrarily set.

