Self-organized criticality in the substorm phenomenon and its relation to localized reconnection in the magnetospheric plasma sheet
Author
dc.contributor.author
Klimas, A. J.
Author
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Valdivia Hepp, Juan
Author
dc.contributor.author
Vassiliadis, D.
Author
dc.contributor.author
Baker, D. N.
Author
dc.contributor.author
Hesse, M.
Author
dc.contributor.author
Takalo, J.
Admission date
dc.date.accessioned
2018-12-20T14:11:46Z
Available date
dc.date.available
2018-12-20T14:11:46Z
Publication date
dc.date.issued
2000
Cita de ítem
dc.identifier.citation
Journal of Geophysical Research: Space Physics, Volumen 105, Issue A8, 2018, Pages 18765-18780
Identifier
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21699402
Identifier
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https://repositorio.uchile.cl/handle/2250/154633
Abstract
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Evidence is presented that suggests that there is a significant self-organized criticality (SOC) component in the dynamics of substorms in the magnetosphere. We assume that observations of bursty bulk flows, fast flows, localized dipolarizations, plasma turbulence, etc. show that multiple localized reconnection sites provide the basic avalanche phenomenon in the establishment of SOC in the plasma sheet. First results are presented from a study of this avalanche process based on this working assumption. A magnetic field reversal model is discussed. Resistivity, in this model, is self-consistently generated in response to the excitation of an idealized current-driven instability. When forced by convection of magnetic flux into the field reversal region, the model yields rapid magnetic field annihilation through a dynamic behavior that is shown to exhibit many of the characteristics of SOC. Over a large range of forcing strengths, the annihilation rate is shown to self-adjust to balance t
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